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\u00a9 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
\n\nWe appreciate the support of the NSF Physics Frontiers Center Award PFC-1430284 and the NSF Physics Frontiers Center Award PFC-2020265. L.B. acknowledges support from the National Science Foundation under award AST-1909933 and from the Research Corporation for Science Advancement under Cottrell Scholar Award No. 27553. P.R.B. is supported by the Science and Technology Facilities Council, grant No. ST/W000946/1. S.B. gratefully acknowledges the support of a Sloan Fellowship and the support of NSF under award #1815664. M.C. and S.R.T. acknowledge support from NSF AST-2007993. M.C. and N.S.P. were supported by the Vanderbilt Initiative in Data Intensive Astrophysics (VIDA) Fellowship. K.Ch., A.D.J., and M.V. acknowledge support from the Caltech and Jet Propulsion Laboratory President's and Director's Research and Development Fund. K.Ch. and A.D.J. acknowledge support from the Sloan Foundation. Support for this work was provided by the NSF through the Grote Reber Fellowship Program administered by Associated Universities, Inc./National Radio Astronomy Observatory. Support for H.T.C. is provided by NASA through the NASA Hubble Fellowship Program grant #HST-HF2-51453.001 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. Pulsar research at UBC is supported by an NSERC Discovery Grant and by CIFAR. K.Cr. is supported by a UBC Four Year Fellowship (6456). M.E.D. acknowledges support from the Naval Research Laboratory by NASA under contract S-15633Y. T.D. and M.T.L. are supported by an NSF Astronomy and Astrophysics Grant (AAG) award number 2009468. E.C.F. is supported by NASA under award number 80GSFC21M0002. G.E.F., S.C.S., and S.J.V. are supported by NSF award PHY-2011772. The Flatiron Institute is supported by the Simons Foundation. S.H. is supported by the National Science Foundation Graduate Research Fellowship under grant No. DGE-1745301. The work of N.La. and X.S. is partly supported by the George and Hannah Bolinger Memorial Fund in the College of Science at Oregon State University. N.La. acknowledges the support from Larry W. Martin and Joyce B. O'Neill Endowed Fellowship in the College of Science at Oregon State University. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). D.R.L. and M.A.M. are supported by NSF #1458952. M.A.M. is supported by NSF #2009425. C.M.F.M. was supported in part by the National Science Foundation under grant Nos. NSF PHY-1748958 and AST-2106552. A.Mi. is supported by the Deutsche Forschungsgemeinschaft under Germany's Excellence Strategy\u2014EXC 2121 Quantum Universe\u2014390833306. The Dunlap Institute is funded by an endowment established by the David Dunlap family and the University of Toronto. K.D.O. was supported in part by NSF grant No. 2207267. T.T.P. acknowledges support from the Extragalactic Astrophysics Research Group at E\u00f6tv\u00f6s Lor\u00e1nd University, funded by the E\u00f6tv\u00f6s Lor\u00e1nd Research Network (ELKH), which was used during the development of this research. S.M.R. and I.H.S. are CIFAR Fellows. Portions of this work performed at NRL were supported by ONR 6.1 basic research funding. J.D.R. also acknowledges support from start-up funds from Texas Tech University. J.S. is supported by an NSF Astronomy and Astrophysics Postdoctoral Fellowship under award AST-2202388, and acknowledges previous support by the NSF under award 1847938. S.R.T. acknowledges support from an NSF CAREER award #2146016. C.U. acknowledges support from BGU (Kreitman fellowship), and the Council for Higher Education and Israel Academy of Sciences and Humanities (Excellence fellowship). C.A.W. acknowledges support from CIERA, the Adler Planetarium, and the Brinson Foundation through a CIERA-Adler postdoctoral fellowship. O.Y. is supported by the National Science Foundation Graduate Research Fellowship under grant No. DGE-2139292.
\n\nenterprise (Ellis et al. 2019), enterprise_extensions (Taylor et al. 2021), QuickCW (B\u00e9csy et al. 2023), corner (Foreman-Mackey 2016), libstempo (Vallisneri 2020), tempo (Nice et al. 2015), tempo2 (Hobbs et al. 2006), PINT (Luo et al. 2019), matplotlib (Hunter 2007), astropy (Astropy Collaboration et al. 2013; Price-Whelan et al. 2018)
", "abstract": "Analyses of pulsar timing data have provided evidence for a stochastic gravitational wave background in the nanohertz frequency band. The most plausible source of this background is the superposition of signals from millions of supermassive black hole binaries. The standard statistical techniques used to search for this background and assess its significance make several simplifying assumptions, namely (i) Gaussianity, (ii) isotropy, and most often, (iii) a power-law spectrum. However, a stochastic background from a finite collection of binaries does not exactly satisfy any of these assumptions. To understand the effect of these assumptions, we test standard analysis techniques on a large collection of realistic simulated data sets. The data-set length, observing schedule, and noise levels were chosen to emulate the NANOGrav 15 yr data set. Simulated signals from millions of binaries drawn from models based on the Illustris cosmological hydrodynamical simulation were added to the data. We find that the standard statistical methods perform remarkably well on these simulated data sets, even though their fundamental assumptions are not strictly met. They are able to achieve a confident detection of the background. However, even for a fixed set of astrophysical parameters, different realizations of the universe result in a large variance in the significance and recovered parameters of the background. We also find that the presence of loud individual binaries can bias the spectral recovery of the background if we do not account for them.
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G." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Wooley-R", "name": { "family": "Wooley", "given": "R." } }, { "id": "Worden-J", "name": { "family": "Worden", "given": "J." } }, { "id": "Yakushin-I", "name": { "family": "Yakushin", "given": "I." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yamamoto-K", "name": { "family": "Yamamoto", "given": "K." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Yoshida-S", "name": { "family": "Yoshida", "given": "S." } }, { "id": "Yu-P-P", "name": { "family": "Yu", "given": "P. P." } }, { "id": "Yvert-M", "name": { "family": "Yvert", "given": "M." } }, { "id": "Zanolin-M", "name": { "family": "Zanolin", "given": "M." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zhang-Zhicai", "name": { "family": "Zhang", "given": "Z." }, "orcid": "0000-0002-1630-0986" }, { "id": "Zhao-Chunnong", "name": { "family": "Zhao", "given": "C." }, "orcid": "0000-0001-5825-2401" }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Belczynski-K", "name": { "family": "Belczynski", "given": "K." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Sensitivity to Gravitational Waves from Compact Binary Coalescences Achieved during LIGO's Fifth and Virgo's First Science Run", "ispublished": "unpub", "full_text_status": "public", "note": "Version history: [v1] Fri, 12 Mar 2010 05:48:36 UTC (403 KB). [v2] Sun, 28 Mar 2010 22:46:53 UTC (403 KB). [v3] Tue, 1 Jun 2010 04:45:05 UTC (403 KB)\n\nSubmitted - 1003_2481.pdf
", "abstract": "We summarize the sensitivity achieved by the LIGO and Virgo gravitational wave detectors for compact binary coalescence (CBC) searches during LIGO's fifth science run and Virgo's first science run. We present noise spectral density curves for each of the four detectors that operated during these science runs which are representative of the typical performance achieved by the detectors for CBC searches. These spectra are intended for release to the public as a summary of detector performance for CBC searches during these science runs.", "date": "2023-09-26", "date_type": "published", "publisher": "California Institute of Technology", "id_number": "CaltechAUTHORS:20230926-170843564", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20230926-170843564", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "other_numbering_system": { "items": [ { "id": "VIR-0171A-10", "name": "Virgo report" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "doi": "10.48550/arXiv.1003.2481", "primary_object": { "basename": "1003_2481.pdf", "url": "https://authors.library.caltech.edu/records/p0b8n-tm695/files/1003_2481.pdf" }, "resource_type": "monograph", "pub_year": "2023", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/yzv7t-bt322", "eprint_id": 105351, "eprint_status": "archive", "datestamp": "2023-08-22 06:23:12", "lastmod": "2023-10-20 21:53:42", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Arzoumanian-Z", "name": { "family": "Arzoumanian", "given": "Zaven" } }, { "name": { "family": "Baker", "given": "Paul T." }, "orcid": "0000-0003-2745-753X" }, { "name": { "family": "Brazier", "given": "Adam" } }, { "name": { "family": "Brook", "given": "Paul R." }, "orcid": "0000-0003-3053-6538" }, { "name": { "family": "Burke-Spolaor", "given": "Sarah" }, "orcid": "0000-0003-4052-7838" }, { "name": { "family": "B\u00e9csy", "given": "Bence" }, "orcid": "0000-0003-0909-5563" }, { "id": "Charisi-M", "name": { "family": "Charisi", "given": "Maria" }, "orcid": "0000-0003-3579-2522" }, { "name": { "family": "Chatterjee", "given": "Shami" }, "orcid": "0000-0002-2878-1502" }, { "name": { "family": "Cordes", "given": "James M." }, "orcid": "0000-0002-4049-1882" }, { "name": { "family": "Cornish", "given": "Neil J." }, "orcid": "0000-0002-7435-0869" }, { "name": { "family": "Crawford", "given": "Fronefield" }, "orcid": "0000-0002-2578-0360" }, { "name": { "family": "Cromartie", "given": "H. Thankful" }, "orcid": "0000-0002-6039-692X" }, { "name": { "family": "Crowter", "given": "Kathryn" }, "orcid": "0000-0002-1529-5169" }, { "name": { "family": "DeCesar", "given": "Megan E." }, "orcid": "0000-0002-2185-1790" }, { "name": { "family": "Demorest", "given": "Paul B." }, "orcid": "0000-0002-6664-965X" }, { "name": { "family": "Dolch", "given": "Timothy" }, "orcid": "0000-0001-8885-6388" }, { "name": { "family": "Elliott", "given": "Rodney D." } }, { "name": { "family": "Ellis", "given": "Justin A." } }, { "name": { "family": "Ferdman", "given": "Robert D." }, "orcid": "0000-0002-2223-1235" }, { "name": { "family": "Ferrara", "given": "Elizabeth C." }, "orcid": "0000-0001-7828-7708" }, { "name": { "family": "Fonseca", "given": "Emmanuel" }, "orcid": "0000-0001-8384-5049" }, { "name": { "family": "Garver-Daniels", "given": "Nathan" }, "orcid": "0000-0001-6166-9646" }, { "name": { "family": "Gentile", "given": "Peter A." }, "orcid": "0000-0001-8158-683X" }, { "name": { "family": "Good", "given": "Deborah C." }, "orcid": "0000-0003-1884-348X" }, { "name": { "family": "Hazboun", "given": "Jeffrey S." }, "orcid": "0000-0003-2742-3321" }, { "name": { "family": "Islo", "given": "Kristina" } }, { "name": { "family": "Jennings", "given": "Ross J." }, "orcid": "0000-0003-1082-2342" }, { "name": { "family": "Jones", "given": "Megan L." }, "orcid": "0000-0001-6607-3710" }, { "name": { "family": "Kaiser", "given": "Andrew R." }, "orcid": "0000-0002-3654-980X" }, { "name": { "family": "Kaplan", "given": "David L." }, "orcid": "0000-0001-6295-2881" }, { "name": { "family": "Kelley", "given": "Luke Zoltan" }, "orcid": "0000-0002-6625-6450" }, { "name": { "family": "Key", "given": "Joey Shapiro" }, "orcid": "0000-0003-0123-7600" }, { "name": { "family": "Lam", "given": "Michael T." }, "orcid": "0000-0003-0721-651X" }, { "id": "Lazio-T-J-W", "name": { "family": "Lazio", "given": "T. Joseph W." }, "orcid": "0000-0002-3873-5497" }, { "name": { "family": "Levin", "given": "Lina" }, "orcid": "0000-0002-2034-2986" }, { "name": { "family": "Luo", "given": "Jing" }, "orcid": "0000-0001-5373-5914" }, { "name": { "family": "Lynch", "given": "Ryan S." }, "orcid": "0000-0001-5229-7430" }, { "name": { "family": "Madison", "given": "Dustin R." }, "orcid": "0000-0003-2285-0404" }, { "name": { "family": "McLaughlin", "given": "Maura A." }, "orcid": "0000-0001-7697-7422" }, { "name": { "family": "Mingarelli", "given": "Chiara M. F." }, "orcid": "0000-0002-4307-1322" }, { "name": { "family": "Ng", "given": "Cherry" }, "orcid": "0000-0002-3616-5160" }, { "name": { "family": "Nice", "given": "David J." }, "orcid": "0000-0002-6709-2566" }, { "name": { "family": "Pennucci", "given": "Timothy T." }, "orcid": "0000-0001-5465-2889" }, { "name": { "family": "Pol", "given": "Nihan S." }, "orcid": "0000-0002-8826-1285" }, { "name": { "family": "Ransom", "given": "Scott M." }, "orcid": "0000-0001-5799-9714" }, { "name": { "family": "Ray", "given": "Paul S." }, "orcid": "0000-0002-5297-5278" }, { "name": { "family": "Shapiro-Albert", "given": "Brent J." }, "orcid": "0000-0002-7283-1124" }, { "name": { "family": "Siemens", "given": "Xavier" }, "orcid": "0000-0002-7778-2990" }, { "id": "Simon-Joseph", "name": { "family": "Simon", "given": "Joseph" }, "orcid": "0000-0003-1407-6607" }, { "name": { "family": "Spiewak", "given": "Ren\u00e9e" }, "orcid": "0000-0002-6730-3298" }, { "name": { "family": "Stairs", "given": "Ingrid H." }, "orcid": "0000-0001-9784-8670" }, { "name": { "family": "Stinebring", "given": "Daniel R." }, "orcid": "0000-0002-1797-3277" }, { "name": { "family": "Stovall", "given": "Kevin" }, "orcid": "0000-0002-7261-594X" }, { "name": { "family": "Swiggum", "given": "Joseph K." }, "orcid": "0000-0002-1075-3837" }, { "name": { "family": "Taylor", "given": "Stephen R." }, "orcid": "0000-0003-0264-1453" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" }, { "name": { "family": "Vigeland", "given": "Sarah J." }, "orcid": "0000-0003-4700-9072" }, { "name": { "family": "Witt", "given": "Caitlin A." }, "orcid": "0000-0002-6020-9274" }, { "name": { "family": "Zhu", "given": "Weiwei" }, "orcid": "0000-0001-5105-4058" } ] }, "title": "Multimessenger Gravitational-wave Searches with Pulsar Timing Arrays: Application to 3C 66B Using the NANOGrav 11-year Data Set", "ispublished": "pub", "full_text_status": "public", "keywords": "Gravitational waves; Pulsars; Astronomy data analysis; Active galactic nuclei", "note": "\u00a9 2020. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. \n\nReceived 2020 May 14; revised 2020 July 22; accepted 2020 July 31; published 2020 September 7. \n\nS.B.S. and C.A.W. were supported in this work by NSF award Nos. 1458952 and 1815664. The NANOGrav collaboration is supported by NSF Physics Frontier Center award No. 1430284. C.A.W. acknowledges support from West Virginia University through the Outstanding Merit Fellowship for Continuing Doctoral Students. S.B.S. is a CIFAR Azrieli Global Scholar in the Gravity and the Extreme Universe program. This research made use of the Super Computing System (Spruce Knob) at WVU, which is funded in part by the National Science Foundation EPSCoR Research Infrastructure Improvement Cooperative Agreement No. 1003907, the state of West Virginia (WVEPSCoR via the Higher Education Policy Commission), and WVU. We acknowledge the use of Thorny Flat at WVU, which is funded in part by National Science Foundation Major Research Instrumentation Program (MRI) award No. 1726534 and WVU. NANOGrav research at UBC is supported by an NSERC Discovery Grant and Discovery Accelerator Supplement and the Canadian Institute for Advanced Research. M.V. and J.S. acknowledge support from the JPL RTD program. S.R.T. was partially supported by an appointment to the NASA Postdoctoral Program at JPL, administered by Oak Ridge Associated Universities through a contract with NASA. J.A.E. was partially supported by NASA through Einstein Fellowship grants PF4-150120. Portions of this work performed at NRL are supported by the Chief of Naval Research. The Flatiron Institute is supported by the Simons Foundation. Portions of this research were carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. Data for this project were collected using the facilities of the Green Bank Observatory and the Arecibo Observatory. The Green Bank Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. The Arecibo Observatory is a facility of the National Science Foundation operated under cooperative agreement by the University of Central Florida in alliance with Yang Enterprises, Inc., and Universidad Metropolitana. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work made use of the online cosmology calculator tool (Wright 2006). We also acknowledge use of numpy (Oliphant 2006), scipy (Virtanen et al. 2020), matplotlib (Hunter 2007), and astropy (Price-Whelan et al. 2018). This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. \n\nAuthor contributions. We list specific contributions to this paper as follows. C.A.W. led the work on this paper, ran the GW searches, and led the development of the manuscript. J.S., S.R.T., S.J.V., and S.B.S. provided guidance throughout the project and key development of the project motivation and scientific interpretation. J.A.E., S.R.T., P.T.B., S.J.V., and C.A.W. designed and implemented the Bayesian search algorithms in enterprise. J.S.H. performed and interpreted the S/N simulations with hasasia. R.D.E. performed initial literature reviews on 3C 66B. N.J.C., J.S.H., D.L.K., M.T.L., T.J.W.L., M.A.M., C.M.F.M., and D.J.N. contributed valuable scientific comments. The NANOGrav data are the result of the work of dozens of people over the course of more than 13 years. Z.A., K.C., P.B.D., M.E.D., T.D., J.A.E., E.C.F., R.D.F., E.F., P.A.G., M.L.J., M.T.L., R.S.L., M.A.M., C.N., D.J.N., T.T.P., S.M.R., P.S.R., R.S., I.H.S., K.S., J.K.S., and W.Z. developed the 11-year data set. All authors are key contributing members of the NANOGrav collaboration.\n\nPublished - Arzoumanian_2020_ApJ_900_102.pdf
", "abstract": "When galaxies merge, the supermassive black holes in their centers may form binaries and emit low-frequency gravitational radiation in the process. In this paper, we consider the galaxy 3C 66B, which was used as the target of the first multimessenger search for gravitational waves. Due to the observed periodicities present in the photometric and astrometric data of the source, it has been theorized to contain a supermassive black hole binary. Its apparent 1.05-year orbital period would place the gravitational-wave emission directly in the pulsar timing band. Since the first pulsar timing array study of 3C 66B, revised models of the source have been published, and timing array sensitivities and techniques have improved dramatically. With these advances, we further constrain the chirp mass of the potential supermassive black hole binary in 3C 66B to less than (1.65 \u00b1 0.02) \u00d7 10\u2079 M_\u2299 using data from the NANOGrav 11-year data set. This upper limit provides a factor of 1.6 improvement over previous limits and a factor of 4.3 over the first search done. Nevertheless, the most recent orbital model for the source is still consistent with our limit from pulsar timing array data. In addition, we are able to quantify the improvement made by the inclusion of source properties gleaned from electromagnetic data over \"blind\" pulsar timing array searches. With these methods, it is apparent that it is not necessary to obtain exact a priori knowledge of the period of a binary to gain meaningful astrophysical inferences.", "date": "2020-09-10", "date_type": "published", "publication": "Astrophysical Journal", "volume": "900", "number": "2", "publisher": "American Astronomical Society", "pagerange": "Art. No. 102", "id_number": "CaltechAUTHORS:20200911-133137947", "issn": "1538-4357", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200911-133137947", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "OIA-1458952" }, { "agency": "NSF", "grant_number": "AST-1815664" }, { "agency": "NSF", "grant_number": "PHY-1430284" }, { "agency": "West Virginia University" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "NSF", "grant_number": "OIA-1003907" }, { "agency": "NSF", "grant_number": "OAC-1726534" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "JPL Research and Technology Development Fund" }, { "agency": "NASA Postdoctoral Program" }, { "agency": "NASA Einstein Fellowship", "grant_number": "PF4-150120" }, { "agency": "Chief of Naval Research" }, { "agency": "Flatiron Institute" }, { "agency": "Simons Foundation" }, { "agency": "NASA/JPL/Caltech" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "NANOGrav Collaboration" ] }, "doi": "10.3847/1538-4357/ababa1", "primary_object": { "basename": "Arzoumanian_2020_ApJ_900_102.pdf", "url": "https://authors.library.caltech.edu/records/yzv7t-bt322/files/Arzoumanian_2020_ApJ_900_102.pdf" }, "resource_type": "article", "pub_year": "2020", "author_list": "Arzoumanian, Zaven; Baker, Paul T.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/t68xc-7qd65", "eprint_id": 101499, "eprint_status": "archive", "datestamp": "2023-08-22 04:04:18", "lastmod": "2023-10-19 22:48:17", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Hazboun-J-S", "name": { "family": "Hazboun", "given": "J. S." }, "orcid": "0000-0003-2742-3321" }, { "id": "Simon-J", "name": { "family": "Simon", "given": "J." }, "orcid": "0000-0003-1407-6607" }, { "id": "Taylor-S-R", "name": { "family": "Taylor", "given": "S. R." }, "orcid": "0000-0003-0264-1453" }, { "name": { "family": "Lam", "given": "M. T." }, "orcid": "0000-0003-0721-651X" }, { "name": { "family": "Vigeland", "given": "S. J." }, "orcid": "0000-0003-4700-9072" }, { "name": { "family": "Islo", "given": "K." }, "orcid": "0000-0001-5123-9917" }, { "name": { "family": "Key", "given": "J. S." }, "orcid": "0000-0003-0123-7600" }, { "name": { "family": "Arzoumanian", "given": "Z." } }, { "name": { "family": "Baker", "given": "P. T." }, "orcid": "0000-0003-2745-753X" }, { "name": { "family": "Brazier", "given": "A." } }, { "name": { "family": "Brook", "given": "P. R." }, "orcid": "0000-0003-3053-6538" }, { "name": { "family": "Burke-Spolaor", "given": "S." }, "orcid": "0000-0003-4052-7838" }, { "name": { "family": "Chatterjee", "given": "S." }, "orcid": "0000-0002-2878-1502" }, { "name": { "family": "Cordes", "given": "J. M." }, "orcid": "0000-0002-4049-1882" }, { "name": { "family": "Cornish", "given": "N. J." }, "orcid": "0000-0002-7435-0869" }, { "name": { "family": "Crawford", "given": "F." }, "orcid": "0000-0002-2578-0360" }, { "name": { "family": "Crowter", "given": "K." }, "orcid": "0000-0002-1529-5169" }, { "name": { "family": "Cromartie", "given": "H. T." }, "orcid": "0000-0002-6039-692X" }, { "name": { "family": "DeCesar", "given": "M." }, "orcid": "0000-0002-2185-1790" }, { "name": { "family": "Demorest", "given": "P. B." }, "orcid": "0000-0002-6664-965X" }, { "name": { "family": "Dolch", "given": "T." }, "orcid": "0000-0001-8885-6388" }, { "name": { "family": "Ellis", "given": "J. A." } }, { "name": { "family": "Ferdman", "given": "R. D." }, "orcid": "0000-0002-2223-1235" }, { "name": { "family": "Ferrara", "given": "E." } }, { "name": { "family": "Fonseca", "given": "E." }, "orcid": "0000-0001-8384-5049" }, { "name": { "family": "Garver-Daniels", "given": "N." }, "orcid": "0000-0001-6166-9646" }, { "name": { "family": "Gentile", "given": "P." }, "orcid": "0000-0001-8158-683X" }, { "name": { "family": "Good", "given": "D." }, "orcid": "0000-0003-1884-348X" }, { "name": { "family": "Holgado", "given": "A. M." }, "orcid": "0000-0003-4143-8132" }, { "name": { "family": "Huerta", "given": "E. A." }, "orcid": "0000-0002-9682-3604" }, { "name": { "family": "Jennings", "given": "R." }, "orcid": "0000-0003-1082-2342" }, { "name": { "family": "Jones", "given": "G." } }, { "name": { "family": "Jones", "given": "M. L." }, "orcid": "0000-0001-6607-3710" }, { "name": { "family": "Kaiser", "given": "A. R." }, "orcid": "0000-0002-3654-980X" }, { "name": { "family": "Kaplan", "given": "D. L." }, "orcid": "0000-0001-6295-2881" }, { "name": { "family": "Kelley", "given": "L. Z." }, "orcid": "0000-0002-6625-6450" }, { "id": "Lazio-T-J-W", "name": { "family": "Lazio", "given": "T. J. W." }, "orcid": "0000-0002-3873-5497" }, { "name": { "family": "Levin", "given": "L." }, "orcid": "0000-0002-2034-2986" }, { "name": { "family": "Lommen", "given": "A. N." }, "orcid": "0000-0003-4137-7536" }, { "name": { "family": "Lorimer", "given": "D. R." }, "orcid": "0000-0003-1301-966X" }, { "name": { "family": "Luo", "given": "J." } }, { "name": { "family": "Lynch", "given": "R. S." }, "orcid": "0000-0001-5229-7430" }, { "name": { "family": "Madison", "given": "D. R." }, "orcid": "0000-0003-2285-0404" }, { "name": { "family": "McLaughlin", "given": "M. A." }, "orcid": "0000-0001-7697-7422" }, { "name": { "family": "McWilliams", "given": "S. T." }, "orcid": "0000-0003-2397-8290" }, { "name": { "family": "Mingarelli", "given": "C. M. F." }, "orcid": "0000-0002-4307-1322" }, { "name": { "family": "Ng", "given": "C." }, "orcid": "0000-0002-3616-5160" }, { "name": { "family": "Nice", "given": "D. J." }, "orcid": "0000-0002-6709-2566" }, { "name": { "family": "Pennucci", "given": "T. T." }, "orcid": "0000-0001-5465-2889" }, { "name": { "family": "Pol", "given": "N. S." }, "orcid": "0000-0002-8826-1285" }, { "name": { "family": "Ransom", "given": "S. M." }, "orcid": "0000-0001-5799-9714" }, { "name": { "family": "Ray", "given": "P. S." }, "orcid": "0000-0002-5297-5278" }, { "name": { "family": "Siemens", "given": "X." }, "orcid": "0000-0002-7778-2990" }, { "name": { "family": "Spiewak", "given": "R." }, "orcid": "0000-0002-6730-3298" }, { "name": { "family": "Stairs", "given": "I. H." }, "orcid": "0000-0001-9784-8670" }, { "name": { "family": "Stinebring", "given": "D. R." }, "orcid": "0000-0002-1797-3277" }, { "name": { "family": "Stovall", "given": "K." }, "orcid": "0000-0002-7261-594X" }, { "name": { "family": "Swiggum", "given": "J." }, "orcid": "0000-0002-1075-3837" }, { "name": { "family": "Turner", "given": "J. E." }, "orcid": "0000-0002-2451-7288" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "van-Haasteren-R", "name": { "family": "van Haasteren", "given": "R." }, "orcid": "0000-0002-6428-2620" }, { "name": { "family": "Witt", "given": "C. A." }, "orcid": "0000-0002-6020-9274" }, { "name": { "family": "Zhu", "given": "W. W." }, "orcid": "0000-0001-5105-4058" } ] }, "title": "NANOGrav 11 yr Data Set: Evolution of Gravitational-wave Background Statistics", "ispublished": "pub", "full_text_status": "public", "keywords": "Millisecond pulsars; Pulsar timing method; Radio pulsars; Red noise; Gravitational waves; Gravitational wave detectors", "note": "\u00a9 2020 The American Astronomical Society. \n\nReceived 2019 September 18; revised 2019 December 24; accepted 2020 January 6; published 2020 February 18. \n\nAuthor contributions. This paper is the result of the work of dozens of people over the course of more than 13 years. We list specific contributions below. J.S.H. ran the sliced analyses and led the paper writing. J.S., S.R.T., M.T.L., S.J.V, K.I., and J.S.K. contributed substantially to paper writing, discussion, and interpretation of results. M.T.L. helped with analyses. J.S.H. and S.R.T. developed the formalism in Section 4. Z.A., K.C., P.B.D., M.E.D., T.D., J.A.E., E.C.F., R.D.F., E.F., P.A.G., G.J., M.L.J., M.T.L., L.L., D.R.L., R.S.L., M.A.M., C.N., D.J.N., T.T.P., S.M.R., P.S.R., R.S., I.H.S., K.S., J.K.S., and W.Z. ran observations and developed the 11 yr data set. \n\nThe NANOGrav project receives support from National Science Foundation (NSF) PIRE program award No. 0968296 and NSF Physics Frontier Center award No. 1430284. NANOGrav research at UBC is supported by an NSERC Discovery Grant and Discovery Accelerator Supplement and by the Canadian Institute for Advanced Research. J.S.H. would like to thank Joseph Romano for a number of in-depth discussions concerning the results of the numerous analyses done for this project. M.V. and J.S. acknowledge support from the JPL RTD program. Portions of this research were carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. S.R.T. was partially supported by an appointment to the NASA Postdoctoral Program at the Jet Propulsion Laboratory, administered by Oak Ridge Associated Universities through a contract with NASA. S.R.T. thanks ERS for fruitful discussions. J.A.E. was partially supported by NASA through Einstein Fellowship grants PF4-150120. S.B.S. was supported by NSF award No. 1458952. P.T.B. acknowledges support from the West Virginia University Center for Gravitational Waves and Cosmology. This work was supported in part by National Science Foundation grant No. PHYS-1066293 and by the hospitality of the Aspen Center for Physics. Portions of this work performed at NRL are supported by the Chief of Naval Research. This research was performed in part using the Zwicky computer cluster at Caltech supported by NSF under MRI-R2 award No. PHY-0960291 and by the Sherman Fairchild Foundation. A majority of the computational work was performed on the Nemo cluster at UWM supported by NSF grant No. 0923409. Parts of the analysis in this work were carried out on the Nimrod cluster made available by S.M.R. Data for this project were collected using the facilities of the National Radio Astronomy Observatory and the Arecibo Observatory. The National Radio Astronomy Observatory and Green Bank Observatory are facilities of the NSF operated under cooperative agreement by Associated Universities, Inc. The Arecibo Observatory is operated by the University of Central Florida, Ana G. M\u00e9ndez-Universidad Metropolitana, and Yang Enterprises under a cooperative agreement with the NSF (AST-1744119). This research is part of the Blue Waters sustained-petascale computing project, which is supported by the National Science Foundation (awards OCI-0725070 and ACI-1238993) and the state of Illinois. Blue Waters is a joint effort of the University of Illinois at Urbana-Champaign and its National Center for Supercomputing Applications. Some of the algorithms used in this article were optimized using the Blue Waters allocation \"Accelerating the detection of gravitational waves with GPUs.\" The Flatiron Institute is supported by the Simons Foundation. \n\nSoftware: enterprise (Ellis et al. 2017), PTMCMCSampler (Ellis & van Haasteren 2017), enterprise_extensions (Taylor et al. 2018), TEMPO2 (Hobbs et al. 2006), libstempo (Vallisneri 2015), Scipy (Jones) and Numpy (Oliphant).\n\nPublished - Hazboun_2020_ApJ_890_108.pdf
", "abstract": "An ensemble of inspiraling supermassive black hole binaries should produce a stochastic background of very low frequency gravitational waves. This stochastic background is predicted to be a power law, with a gravitational-wave strain spectral index of \u22122/3, and it should be detectable by a network of precisely timed millisecond pulsars, widely distributed on the sky. This paper reports a new \"time slicing\" analysis of the 11 yr data release from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) using 34 millisecond pulsars. Methods to flag potential \"false-positive\" signatures are developed, including techniques to identify responsible pulsars. Mitigation strategies are then presented. We demonstrate how an incorrect noise model can lead to spurious signals, and we show how independently modeling noise across 30 Fourier components, spanning NANOGrav's frequency range, effectively diagnoses and absorbs the excess power in gravitational-wave searches. This results in a nominal, and expected, progression of our gravitational-wave statistics. Additionally, we show that the first interstellar medium event in PSR J1713+0747 pollutes the common red-noise process with low spectral index noise, and we use a tailored noise model to remove these effects.", "date": "2020-02-20", "date_type": "published", "publication": "Astrophysical Journal", "volume": "890", "number": "2", "publisher": "American Astronomical Society", "pagerange": "Art. No. 108", "id_number": "CaltechAUTHORS:20200224-125802735", "issn": "1538-4357", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200224-125802735", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "OISE-0968296" }, { "agency": "NSF", "grant_number": "PHY-1430284" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "JPL Research and Technology Development Fund" }, { "agency": "NASA/JPL/Caltech" }, { "agency": "NASA Postdoctoral Program" }, { "agency": "NASA Einstein Fellowship", "grant_number": "PF4-150120" }, { "agency": "NSF", "grant_number": "OIA-1458952" }, { "agency": "West Virginia University" }, { "agency": "NSF", "grant_number": "PHYS-1066293" }, { "agency": "Chief of Naval Research" }, { "agency": "NSF", "grant_number": "PHY-0960291" }, { "agency": "Sherman Fairchild Foundation" }, { "agency": "NSF", "grant_number": "PHY-0923409" }, { "agency": "NSF", "grant_number": "AST-1744119" }, { "agency": "NSF", "grant_number": "OCI-0725070" }, { "agency": "NSF", "grant_number": "ACI-1238993" }, { "agency": "State of Illinois" }, { "agency": "Simons Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "NANOGrav Collaboration" ] }, "doi": "10.3847/1538-4357/ab68db", "primary_object": { "basename": "Hazboun_2020_ApJ_890_108.pdf", "url": "https://authors.library.caltech.edu/records/t68xc-7qd65/files/Hazboun_2020_ApJ_890_108.pdf" }, "resource_type": "article", "pub_year": "2020", "author_list": "Hazboun, J. S.; Simon, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/dwr02-p7076", "eprint_id": 97548, "eprint_status": "archive", "datestamp": "2023-08-19 17:12:25", "lastmod": "2023-10-18 16:04:38", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aggarwal-K", "name": { "family": "Aggarwal", "given": "K." } }, { "id": "Simon-J", "name": { "family": "Simon", "given": "J." }, "orcid": "0000-0003-1407-6607" }, { "id": "Taylor-S-R", "name": { "family": "Taylor", "given": "S. R." }, "orcid": "0000-0003-0264-1453" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "The NANOGrav 11 yr Data Set: Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2019 The American Astronomical Society. \n\nReceived 2018 December 28; revised 2019 April 17; accepted 2019 May 15; published 2019 July 31. \n\nThis paper is the result of the work of dozens of people over the course of more than 13 years. We list specific contributions below. Z.A., K.C., P.B.D., M.E.D., T.D., J.A.E., E.C.F., R.D.F., E.F., P.A.G., G.J., M.L.J., M.T.L., L.L., D.R.L., R.S.L., M.A.M., C.N., D.J.N., T.T.P., S.M.R., P.S.R., R.S., I.H.S., K.S., J.K.S., and W.Z. developed the 11 yr data set. S.J.V. led the search and coordinated the paper writing. J.A.E., S.R.T., P.T.B., S.J.V., and C.A.W. designed and implemented the Bayesian search algorithms in enterprise, and A.R.K., S.T.M., S.R.T., and S.J.V. implemented the Fp-statistic in enterprise. N.J.C. helped to uncover a bug in an early implementation of the search algorithms. P.T.B. developed the jump proposals based on empirical distributions. S.J.V., K.I., J.E.T., K.A., P.R.B., A.M.H., and N.S.P. ran the searches. M.R.B, J.A.E., and S.R.T. performed an initial analysis of the 9 yr data set. C.M.F.M., K.I., T.J.W.L., J.S., and S.J.V. did the astrophysical interpretation. S.J.V., K.I., and C.M.F.M. wrote the paper and generated the plots. \n\nWe thank the anonymous referee for helpful comments and suggestions that improved this manuscript. The NANOGrav project receives support from National Science Foundation (NSF) Physics Frontier Center award number 1430284. NANOGrav research at UBC is supported by an NSERC Discovery Grant and Discovery Accelerator Supplement and by the Canadian Institute for Advanced Research. Portions of this research were carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. M.V. and J.S. acknowledge support from the JPL RTD program. S.R.T. was partially supported by an appointment to the NASA Postdoctoral Program at the Jet Propulsion Laboratory, administered by Oak Ridge Associated Universities through a contract with NASA. M.A.M., S.B.S., D.R.L., S.T.M., and P.R.B. were supported by NSF award number #1458952. M.A.M. and N.P. were supported by NSF award number #1517003. J.A.E. was partially supported by NASA through Einstein Fellowship grants PF4-150120. S.B.S. and C.A.W. were supported by NSF award #1815664. W.W.Z. is supported by the Chinese Academy of Science Pioneer Hundred Talents Program, the Strategic Priority Research Program of the Chinese Academy of Sciences grant No. XDB23000000, the National Natural Science Foundation of China grant No. 11690024, and by the Astronomical Big Data Joint Research Center, co-founded by the National Astronomical Observatories, Chinese Academy of Sciences and the Alibaba Cloud. Portions of this work performed at N.R.L. are supported by the Chief of Naval Research. The Flatiron Institute is supported by the Simons Foundation. \n\nWe thank Logan O'Beirne for helping to uncover a bug in an early implementation of the search algorithms, and for providing comments on the algorithms and manuscript. We thank Casey McGrath for performing some of the CW analyses. We thank Luke Kelley and Tingting Liu for helpful discussions. We thank Alberto Sesana, Xinjiang Zhu, and Siyuan Chen for providing useful comments on the manuscript. \n\nWe are grateful for computational resources provided by the Leonard E Parker Center for Gravitation, Cosmology and Astrophysics at the University of Wisconsin-Milwaukee, which is supported by NSF Grants 0923409 and 1626190. This research made use of the Super Computing System (Spruce Knob) at WVU, which is funded in part by the National Science Foundation EPSCoR Research Infrastructure Improvement Cooperative Agreement #1003907, the state of West Virginia (WVEPSCoR via the Higher Education Policy Commission) and WVU. This research also made use of the Illinois Campus Cluster, a computing resource that is operated by the Illinois Campus Cluster Program (ICCP) in conjunction with the National Center for Supercomputing Applications (NCSA) and which is supported by funds from the University of Illinois at Urbana-Champaign. Data for this project were collected using the facilities of the Green Bank Observatory and the Arecibo Observatory. The Green Bank Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. The Arecibo Observatory is a facility of the National Science Foundation operated under cooperative agreement by the University of Central Florida in alliance with Yang Enterprises, Inc. and Universidad Metropolitana. \n\nSoftware: enterprise (Ellis et al. 2017), PAL2 (Ellis & van Haasteren 2017a), PTMCMCSampler (Ellis & van Haasteren 2017b).\n\nPublished - Aggarwal_2019_ApJ_880_116.pdf
Accepted Version - 1812.11585.pdf
", "abstract": "Observations indicate that nearly all galaxies contain supermassive black holes at their centers. When galaxies merge, their component black holes form SMBH binaries (SMBHBs), which emit low-frequency gravitational waves (GWs) that can be detected by pulsar timing arrays. We have searched the North American Nanohertz Observatory for Gravitational Waves 11 yr data set for GWs from individual SMBHBs in circular orbits. As we did not find strong evidence for GWs in our data, we placed 95% upper limits on the strength of GWs from such sources. At f_(gw) = 8 nHz, we placed a sky-averaged upper limit of h_0 < 7.3(3) \u00d7 10^(\u221215). We also developed a technique to determine the significance of a particular signal in each pulsar using \"dropout\" parameters as a way of identifying spurious signals. From these upper limits, we ruled out SMBHBs emitting GWs with f_(gw) = 8 nHz within 120 Mpc for M = 10^9 M\u2299, and within 5.5 Gpc for M = 10^(10)M\u2299 at our most sensitive sky location. We also determined that there are no SMBHBs with M > 1.6 x 10^9 M\u2299 emitting GWs with f_(gw) = 2.8\u2013317.8 nHz in the Virgo Cluster. Finally, we compared our strain upper limits to simulated populations of SMBHBs, based on galaxies in the Two Micron All-Sky Survey and merger rates from the Illustris cosmological simulation project, and found that only 34 out of 75,000 realizations of the local universe contained a detectable source.", "date": "2019-08-01", "date_type": "published", "publication": "Astrophysical Journal", "volume": "880", "number": "2", "publisher": "American Astronomical Society", "pagerange": "Art. No. 116", "id_number": "CaltechAUTHORS:20190731-102317556", "issn": "1538-4357", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20190731-102317556", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "PHY-1430284" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "NASA/JPL/Caltech" }, { "agency": "JPL Research and Technology Development Fund" }, { "agency": "NASA Postdoctoral Program" }, { "agency": "NSF", "grant_number": "OIA-1458952" }, { "agency": "NSF", "grant_number": "AST-1517003" }, { "agency": "NASA Einstein Fellowship", "grant_number": "PF4-150120" }, { "agency": "NSF", "grant_number": "AST-1815664" }, { "agency": "Chinese Academy of Sciences", "grant_number": "XDB23000000" }, { "agency": "National Natural Science Foundation of China", "grant_number": "11690024" }, { "agency": "Astronomical Big Data Joint Research Center" }, { "agency": "National Astronomical Observatories, Chinese Academy of Sciences (NAOC)" }, { "agency": "Alibaba Cloud" }, { "agency": "Chief of Naval Research" }, { "agency": "Simons Foundation" }, { "agency": "NSF", "grant_number": "PHY-0923409" }, { "agency": "NSF", "grant_number": "PHY-1626190" }, { "agency": "NSF", "grant_number": "OIA-1003907" }, { "agency": "State of West Virginia" }, { "agency": "West Virginia University" }, { "agency": "University of Illinois Urbana-Champaign" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "NANOGrav Collaboration" ] }, "doi": "10.3847/1538-4357/ab2236", "primary_object": { "basename": "1812.11585.pdf", "url": "https://authors.library.caltech.edu/records/dwr02-p7076/files/1812.11585.pdf" }, "related_objects": [ { "basename": "Aggarwal_2019_ApJ_880_116.pdf", "url": "https://authors.library.caltech.edu/records/dwr02-p7076/files/Aggarwal_2019_ApJ_880_116.pdf" } ], "resource_type": "article", "pub_year": "2019", "author_list": "Aggarwal, K.; Simon, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/ads5c-a0266", "eprint_id": 97929, "eprint_status": "archive", "datestamp": "2023-08-19 17:05:34", "lastmod": "2023-10-18 16:53:35", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Wang-Haochen", "name": { "family": "Wang", "given": "Haochen" } }, { "id": "Taylor-S-R", "name": { "family": "Taylor", "given": "Stephen R." }, "orcid": "0000-0003-0264-1453" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Bayesian cross validation for gravitational-wave searches in pulsar-timing array data", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves \u2013 methods: statistical \u2013 pulsars: general", "note": "\u00a9 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). \n\nAccepted 2019 May 28. Received 2019 May 24; in original form 2019 April 10. Published: 04 June 2019. \n\nWe thank Joseph Simon and Michael Lam for discussions regarding the dispersion-measure variation of PSR J1713+0747. This research was performed in part using the Zwicky computer cluster at Caltech supported by the National Science Foundation under MRI-R2 award No. PHY0960291 and by the Sherman Fairchild Foundation. Portions of this research were carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This work was supported in part by National Science Foundation Grant No. PHYS-1066293 and by the hospitality of the Aspen Center for Physics. MV was supported by the Jet Propulsion Laboratory RTD program. SRT was supported by the NANOGrav National Science Foundation Physics Frontier Center, award number 1430284. Parts of this work were carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract to the National Aeronautics and Space Administration. Copyright 2019 California Institute of Technology. Government sponsorship acknowledged.\n\nPublished - stz1537.pdf
Submitted - 1904.05355.pdf
", "abstract": "Gravitational-wave data analysis demands sophisticated statistical noise models in a bid to extract highly obscured signals from data. In Bayesian model comparison, we choose among a landscape of models by comparing their marginal likelihoods. However, this computation is numerically fraught and can be sensitive to arbitrary choices in the specification of parameter priors. In Bayesian cross validation, we characterize the fit and predictive power of a model by computing the Bayesian posterior of its parameters in a training data set, and then use that posterior to compute the averaged likelihood of a different testing data set. The resulting cross-validation scores are straightforward to compute; they are insensitive to prior tuning; and they penalize unnecessarily complex models that overfit the training data at the expense of predictive performance. In this article, we discuss cross validation in the context of pulsar-timing-array data analysis, and we exemplify its application to simulated pulsar data (where it successfully selects the correct spectral index of a stochastic gravitational-wave background), and to a pulsar data set from the NANOGrav 11-yr release (where it convincingly favours a model that represents a transient feature in the interstellar medium). We argue that cross validation offers a promising alternative to Bayesian model comparison, and we discuss its use for gravitational-wave detection, by selecting or refuting models that include a gravitational-wave component.", "date": "2019-08", "date_type": "published", "publication": "Monthly Notices of the Royal Astronomical Society", "volume": "487", "number": "3", "publisher": "Royal Astronomical Society", "pagerange": "3644-3649", "id_number": "CaltechAUTHORS:20190815-140748905", "issn": "0035-8711", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20190815-140748905", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "PHY-0960291" }, { "agency": "Sherman Fairchild Foundation" }, { "agency": "NASA/JPL/Caltech" }, { "agency": "NSF", "grant_number": "PHYS-1066293" }, { "agency": "JPL Research and Technology Development Fund" }, { "agency": "NSF", "grant_number": "PHY-1430284" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1093/mnras/stz1537", "primary_object": { "basename": "stz1537.pdf", "url": "https://authors.library.caltech.edu/records/ads5c-a0266/files/stz1537.pdf" }, "related_objects": [ { "basename": "1904.05355.pdf", "url": "https://authors.library.caltech.edu/records/ads5c-a0266/files/1904.05355.pdf" } ], "resource_type": "article", "pub_year": "2019", "author_list": "Wang, Haochen; Taylor, Stephen R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/v2q00-0b067", "eprint_id": 86584, "eprint_status": "archive", "datestamp": "2023-08-19 09:19:07", "lastmod": "2023-10-18 19:45:03", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Arzoumanian-Z", "name": { "family": "Arzoumanian", "given": "Z." } }, { "id": "Lazio-T-J-W", "name": { "family": "Lazio", "given": "T. J. W." }, "orcid": "0000-0002-3873-5497" }, { "id": "Taylor-S-R", "name": { "family": "Taylor", "given": "S. R." }, "orcid": "0000-0003-0264-1453" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "The NANOGrav 11 Year Data Set: Pulsar-timing Constraints on the Stochastic Gravitational-wave Background", "ispublished": "pub", "full_text_status": "public", "keywords": "ephemerides \u2013 gravitational waves \u2013 inflation \u2013 methods: data analysis \u2013 pulsars: general \u2013 quasars: supermassive black holes", "note": "\u00a9 2018 The American Astronomical Society. \n\nReceived 2017 December 19; revised 2018 March 31; accepted 2018 April 8; published 2018 May 23. \n\nWe thank the referee for useful suggestions and comments that improved the quality of this manuscript. The NANOGrav project receives support from NSF Physics Frontier Center award number 1430284. NANOGrav research at UBC is supported by an NSERC Discovery Grant and Discovery Accelerator Supplement and by the Canadian Institute for Advanced Research. We thank our colleagues in the International Pulsar Timing Array for comments and useful discussions. We thank Alberto Sesana for commenting on our astrophysical modeling and interpretation. M.V. and J.S. acknowledge support from the JPL RTD program. Portions of this research were carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. S.R.T. was partially supported by an appointment to the NASA Postdoctoral Program at the Jet Propulsion Laboratory, administered by Oak Ridge Associated Universities through a contract with NASA. S.R.T. thanks E.R.S. for fruitful discussions. J.A.E. was partially supported by NASA through Einstein Fellowship grant PF4-150120. S.B.S. was supported by NSF award #1458952. P.T.B. acknowledges support from the West Virginia University Center for Gravitational Waves and Cosmology. M.A.M. was partially supported by NSF award OIA-1458952. W.W.Z. is supported by the CAS Pioneer Hundred Talents Program and the Strategic Priority Research Program of the Chinese Academy of Sciences grant No. XDB23000000. R.v.H. was supported by NASA Einstein Fellowship grant PF3-140116. This work was supported in part by National Science Foundation grant No. PHYS-1066293 and by the hospitality of the Aspen Center for Physics. Portions of this work performed at NRL are supported by the Chief of Naval Research. This research was performed in part using the Zwicky computer cluster at Caltech supported by NSF under MRI-R2 award No. PHY-0960291 and by the Sherman Fairchild Foundation. A majority of the computational work was performed on the Nemo cluster at UWM supported by NSF grant No. 0923409. Parts of the analysis in this work were carried out on the Nimrod cluster made available by S.M.R. Data for this project were collected using the facilities of the National Radio Astronomy Observatory and the Arecibo Observatory. The National Radio Astronomy Observatory is a facility of the NSF operated under cooperative agreement by Associated Universities, Inc. The Green Bank Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. The Arecibo Observatory is operated by SRI International under a cooperative agreement with the NSF (AST-1100968), and in alliance with Ana G. M\u00e9ndez-Universidad Metropolitana and the Universities Space Research Association. This research is part of the Blue Waters sustained-petascale computing project, which is supported by the National Science Foundation (awards OCI-0725070 and ACI-1238993) and the state of Illinois. Blue Waters is a joint effort of the University of Illinois at Urbana-Champaign and its National Center for Supercomputing Applications. Some of the algorithms used in this article were optimized using the Blue Waters allocation \"Accelerating the detection of gravitational waves with GPUs.\" The Flatiron Institute is supported by the Simons Foundation.\n\nPublished - Arzoumanian_2018_ApJ_859_47.pdf
Submitted - 1801.02617.pdf
", "abstract": "We search for an isotropic stochastic gravitational-wave background (GWB) in the newly released 11 year data set from the North American Nanohertz Observatory for Gravitational Waves (NANOGrav). While we find no evidence for a GWB, we place constraints on a population of inspiraling supermassive black hole (SMBH) binaries, a network of decaying cosmic strings, and a primordial GWB. For the first time, we find that the GWB constraints are sensitive to the solar system ephemeris (SSE) model used and that SSE errors can mimic a GWB signal. We developed an approach that bridges systematic SSE differences, producing the first pulsar-timing array (PTA) constraints that are robust against SSE errors. We thus place a 95% upper limit on the GW-strain amplitude of A_(GWB) < 1.45 \u00d7 10^(\u221215) at a frequency of f = 1 yr^(\u22121) for a fiducial f^(\u22122/3) power-law spectrum and with interpulsar correlations modeled. This is a factor of ~2 improvement over the NANOGrav nine-year limit calculated using the same procedure. Previous PTA upper limits on the GWB (as well as their astrophysical and cosmological interpretations) will need revision in light of SSE systematic errors. We use our constraints to characterize the combined influence on the GWB of the stellar mass density in galactic cores, the eccentricity of SMBH binaries, and SMBH\u2013galactic-bulge scaling relationships. We constrain the cosmic-string tension using recent simulations, yielding an SSE-marginalized 95% upper limit of G\u03bc < 5.3 \u00d7 10^(\u221211)\u2014a factor of ~2 better than the published NANOGrav nine-year constraints. Our SSE-marginalized 95% upper limit on the energy density of a primordial GWB (for a radiation-dominated post-inflation universe) is \u03a9_(GWB)(f) h^2 < 3.4 \u00d7 10^(\u221210).", "date": "2018-05-20", "date_type": "published", "publication": "Astrophysical Journal", "volume": "859", "number": "1", "publisher": "American Astronomical Society", "pagerange": "Art. No. 47", "id_number": "CaltechAUTHORS:20180524-093543782", "issn": "1538-4357", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180524-093543782", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "AST-1430284" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "JPL Research and Technology Development Fund" }, { "agency": "NASA/JPL/Caltech" }, { "agency": "NASA Postdoctoral Program" }, { "agency": "NASA Einstein Fellowship", "grant_number": "PF4-150120" }, { "agency": "NSF", "grant_number": "AST-145895" }, { "agency": "West Virginia University" }, { "agency": "NSF", "grant_number": "OIA-1458952" }, { "agency": "Chinese Academy of Sciences", "grant_number": "XDB23000000" }, { "agency": "NASA Einstein Fellowship", "grant_number": "PF3-140116" }, { "agency": "NSF", "grant_number": "PHYS-1066293" }, { "agency": "Chief of Naval Research" }, { "agency": "NSF", "grant_number": "PHY-0960291" }, { "agency": "Sherman Fairchild Foundation" }, { "agency": "NSF", "grant_number": "AST-0923409" }, { "agency": "NSF", "grant_number": "AST-1100968" }, { "agency": "NSF", "grant_number": "OCI-0725070" }, { "agency": "NSF", "grant_number": "ACI-1238993" }, { "agency": "State of Illinois" }, { "agency": "Simons Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "NANOGrav Collaboration" ] }, "doi": "10.3847/1538-4357/aabd3b", "primary_object": { "basename": "1801.02617.pdf", "url": "https://authors.library.caltech.edu/records/v2q00-0b067/files/1801.02617.pdf" }, "related_objects": [ { "basename": "Arzoumanian_2018_ApJ_859_47.pdf", "url": "https://authors.library.caltech.edu/records/v2q00-0b067/files/Arzoumanian_2018_ApJ_859_47.pdf" } ], "resource_type": "article", "pub_year": "2018", "author_list": "Arzoumanian, Z.; Lazio, T. J. W.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/j0sx1-zq322", "eprint_id": 86284, "eprint_status": "archive", "datestamp": "2023-08-19 09:14:16", "lastmod": "2023-10-18 19:26:07", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ananyeva-A", "name": { "family": "Ananyeva", "given": "A." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Appert-S", "name": { "family": "Appert", "given": "S." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Berger-B-K", "name": { "family": "Berger", "given": "B. K." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Brunett-S", "name": { "family": "Brunett", "given": "S." } }, { "id": "Cahillane-C", "name": { "family": "Cahillane", "given": "C." } }, { "id": "Callister-T-A", "name": { "family": "Callister", "given": "T. A." }, "orcid": "0000-0001-9892-177X" }, { "id": "Cepeda-C-B", "name": { "family": "Cepeda", "given": "C. B." } }, { "id": "Couvares-P", "name": { "family": "Couvares", "given": "P." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Eichholz-J", "name": { "family": "Eichholz", "given": "J." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Feicht-J", "name": { "family": "Feicht", "given": "J." } }, { "id": "Fries-E-M", "name": { "family": "Fries", "given": "E. M." } }, { "id": "Gossan-S-E", "name": { "family": "Gossan", "given": "S. E." }, "orcid": "0000-0002-8138-9198" }, { "id": "Gushwa-K-E", "name": { "family": "Gushwa", "given": "K. E." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hall-E-D", "name": { "family": "Hall", "given": "E. D." }, "orcid": "0000-0001-9018-666X" }, { "id": "Heptonstall-A-W", "name": { "family": "Heptonstall", "given": "A. W." } }, { "id": "Isi-M", "name": { "family": "Isi", "given": "M." }, "orcid": "0000-0001-8830-8672" }, { "id": "Kanner-J-B", "name": { "family": "Kanner", "given": "J. B." }, "orcid": "0000-0001-8115-0577" }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Korth-W-Z", "name": { "family": "Korth", "given": "W. Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D. B." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Massinger-T-J", "name": { "family": "Massinger", "given": "T. J." }, "orcid": "0000-0002-3429-5025" }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "McIver-J", "name": { "family": "McIver", "given": "J." }, "orcid": "0000-0003-0316-1355" }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Quintero-E-A", "name": { "family": "Quintero", "given": "E. A." } }, { "id": "Reitze-D-H", "name": { "family": "Reitze", "given": "D. H." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Rollins-J-G", "name": { "family": "Rollins", "given": "J. G." } }, { "id": "Sachdev-S", "name": { "family": "Sachdev", "given": "S." }, "orcid": "0000-0002-2432-7070" }, { "id": "Sanchez-E-J", "name": { "family": "Sanchez", "given": "E. J." } }, { "id": "Schmidt-P", "name": { "family": "Schmidt", "given": "P." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-R-J-E", "name": { "family": "Smith", "given": "R. J. E." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Tso-Rhondale", "name": { "family": "Tso", "given": "R." }, "orcid": "0000-0003-4464-0117" }, { "id": "Urban-A-L", "name": { "family": "Urban", "given": "A. L." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Venugopalan-G", "name": { "family": "Venugopalan", "given": "G." } }, { "id": "Wade-A-R", "name": { "family": "Wade", "given": "A. R." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Blackman-J", "name": { "family": "Blackman", "given": "J." }, "orcid": "0000-0002-7113-0289" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Ma-Yiqiu", "name": { "family": "Ma", "given": "Y." }, "orcid": "0000-0001-7192-4874" }, { "id": "Pang-Belinda-Heyun", "name": { "family": "Pang", "given": "B." }, "orcid": "0000-0002-5697-2162" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Varma-V", "name": { "family": "Varma", "given": "V." }, "orcid": "0000-0002-9994-1761" } ] }, "title": "Constraints on cosmic strings using data from the first Advanced LIGO observing run", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2018 American Physical Society. \n\nReceived 4 December 2017; published 8 May 2018. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Agencia Estatal de Investigaci\u00f3n, the Vicepresid\u00e8ncia i Conselleria d'Innovaci\u00f3, Recerca i Turisme and the Conselleria d'Educaci\u00f3 i Universitat del Govern de les Illes Balears, the Conselleria d'Educaci\u00f3, Investigaci\u00f3, Cultura i Esport de la Generalitat Valenciana, the National Science Centre of Poland, the Swiss National Science Foundation (SNSF), the Russian Foundation for Basic Research, the Russian Science Foundation, the European Commission, the European Regional Development Funds (ERDF), the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research, Development and Innovation Office Hungary (NKFI), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, the Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, Innovations, and Communications, the International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), the Research Grants Council of Hong Kong, the National Natural Science Foundation of China (NSFC), the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS and the State of Niedersachsen/Germany for provision of computational resources. We would like to thank Christophe Ringeval for many useful discussions.\n\nPublished - PhysRevD.97.102002.pdf
Submitted - 1712.01168.pdf
", "abstract": "Cosmic strings are topological defects which can be formed in grand unified theory scale phase transitions in the early universe. They are also predicted to form in the context of string theory. The main mechanism for a network of Nambu-Goto cosmic strings to lose energy is through the production of loops and the subsequent emission of gravitational waves, thus offering an experimental signature for the existence of cosmic strings. Here we report on the analysis conducted to specifically search for gravitational-wave bursts from cosmic string loops in the data of Advanced LIGO 2015-2016 observing run (O1). No evidence of such signals was found in the data, and as a result we set upper limits on the cosmic string parameters for three recent loop distribution models. In this paper, we initially derive constraints on the string tension \nG\n\u03bc\n and the intercommutation probability, using not only the burst analysis performed on the O1 data set but also results from the previously published LIGO stochastic O1 analysis, pulsar timing arrays, cosmic microwave background and big-bang nucleosynthesis experiments. We show that these data sets are complementary in that they probe gravitational waves produced by cosmic string loops during very different epochs. Finally, we show that the data sets exclude large parts of the parameter space of the three loop distribution models we consider.", "date": "2018-05-15", "date_type": "published", "publication": "Physical Review D", "volume": "97", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102002", "id_number": "CaltechAUTHORS:20180508-132138534", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180508-132138534", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Foundation for Fundamental Research on Matter" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Agencia Estatal de Investigaci\u00f3n" }, { "agency": "Vicepresid\u00e8ncia i Conselleria d'Innovaci\u00f3, Recerca i Turisme" }, { "agency": "Conselleria d'Educaci\u00f3 i Universitat del Govern de les Illes Balears" }, { "agency": "Conselleria d'Educaci\u00f3, Investigaci\u00f3, Cultura i Esport de la Generalitat Valenciana" }, { "agency": "National Science Centre (Poland)" }, { "agency": "Swiss National Science Foundation (SNSF)" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Russian Science Foundation" }, { "agency": "European Commission" }, { "agency": "European Regional Development Fund" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research, Development and Innovation Office (Hungary)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Science and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia, Inova\u00e7\u00e3o e Comunica\u00e7\u00e3o (MCTIC)" }, { "agency": "International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR)" }, { "agency": "Research Grants Council of Hong Kong" }, { "agency": "National Natural Science Foundation of China" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "Astronomy-Department" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.97.102002", "primary_object": { "basename": "1712.01168.pdf", "url": "https://authors.library.caltech.edu/records/j0sx1-zq322/files/1712.01168.pdf" }, "related_objects": [ { "basename": "PhysRevD.97.102002.pdf", "url": "https://authors.library.caltech.edu/records/j0sx1-zq322/files/PhysRevD.97.102002.pdf" } ], "resource_type": "article", "pub_year": "2018", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/h823x-tes28", "eprint_id": 84994, "eprint_status": "archive", "datestamp": "2023-08-21 22:54:51", "lastmod": "2023-10-18 17:02:40", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Kaplan-D-L", "name": { "family": "Kaplan", "given": "D. L." }, "orcid": "0000-0001-6295-2881" }, { "id": "Swiggum-J-K", "name": { "family": "Swiggum", "given": "J. K." }, "orcid": "0000-0002-1075-3837" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "A Gaussian Mixture Model for Nulling Pulsars", "ispublished": "pub", "full_text_status": "public", "keywords": "methods: data analysis; methods: statistical; pulsars: general", "note": "\u00a9 2018 American Astronomical Society. \n\nReceived 2018 January 4. Accepted 2018 January 26. Published 2018 February 28. \n\nWe thank S. McSweeney for helpful comments. We thank the anonymous referee and the AAS journals statistics editor for their suggestions. The Green Bank Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Support was provided by the NANOGrav NSF Physics Frontiers Center award number 1430284. M.V. acknowledges support from the JPL RTD program. Portions of this research were carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.\n\nPublished - Kaplan_2018_ApJ_855_14.pdf
Submitted - 1801.09598.pdf
", "abstract": "The phenomenon of pulsar nulling\u2014where pulsars occasionally turn off for one or more pulses\u2014provides insight into pulsar-emission mechanisms and the processes by which pulsars turn off when they cross the \"death line.\" However, while ever more pulsars are found that exhibit nulling behavior, the statistical techniques used to measure nulling are biased, with limited utility and precision. In this paper, we introduce an improved algorithm, based on Gaussian mixture models, for measuring pulsar nulling behavior. We demonstrate this algorithm on a number of pulsars observed as part of a larger sample of nulling pulsars, and show that it performs considerably better than existing techniques, yielding better precision and no bias. We further validate our algorithm on simulated data. Our algorithm is widely applicable to a large number of pulsars even if they do not show obvious nulls. Moreover, it can be used to derive nulling probabilities of nulling for individual pulses, which can be used for in-depth studies.", "date": "2018-03-01", "date_type": "published", "publication": "Astrophysical Journal", "volume": "855", "number": "1", "publisher": "American Astronomical Society", "pagerange": "Art. No. 14", "id_number": "CaltechAUTHORS:20180228-093052525", "issn": "1538-4357", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180228-093052525", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "PHY-1430284" }, { "agency": "JPL Research and Technology Development Fund" }, { "agency": "NASA/JPL/Caltech" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.3847/1538-4357/aaab62", "primary_object": { "basename": "1801.09598.pdf", "url": "https://authors.library.caltech.edu/records/h823x-tes28/files/1801.09598.pdf" }, "related_objects": [ { "basename": "Kaplan_2018_ApJ_855_14.pdf", "url": "https://authors.library.caltech.edu/records/h823x-tes28/files/Kaplan_2018_ApJ_855_14.pdf" } ], "resource_type": "article", "pub_year": "2018", "author_list": "Kaplan, D. L.; Swiggum, J. K.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/dz3bq-zaf59", "eprint_id": 84473, "eprint_status": "archive", "datestamp": "2023-08-19 07:25:21", "lastmod": "2023-10-18 16:15:30", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ananyeva-A", "name": { "family": "Ananyeva", "given": "A." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Appert-S", "name": { "family": "Appert", "given": "S." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. 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R." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Blackman-J", "name": { "family": "Blackman", "given": "J." }, "orcid": "0000-0002-7113-0289" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Ma-Yiqiu", "name": { "family": "Ma", "given": "Y." }, "orcid": "0000-0001-7192-4874" }, { "id": "Pang-Belinda-Heyun", "name": { "family": "Pang", "given": "B." }, "orcid": "0000-0002-5697-2162" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Varma-V", "name": { "family": "Varma", "given": "V." }, "orcid": "0000-0002-9994-1761" } ] }, "title": "First Search for Nontensorial Gravitational Waves from Known Pulsars", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2018 American Physical Society. \n\nReceived 12 October 2017; revised manuscript received 16 November 2017; published 19 January 2018. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen, Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3, Cultura i Universitats of the Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, Funda\u00e7ao de Amparo \u00e0 Pesquisa do Estado de S\u00e3o Paulo (FAPESP), Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, Ministry of Science and Technology (MOST), Taiwan, and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, and the State of Niedersachsen, Germany for provision of computational resources. \n\nThis paper has been assigned LIGO Document Number LIGO-P1700009.\n\nPublished - PhysRevLett.120.031104.pdf
Submitted - 1709.09203.pdf
Supplemental Material - cwpols_o1_tables.pdf
", "abstract": "We present results from the first directed search for nontensorial gravitational waves. While general relativity allows for tensorial (plus and cross) modes only, a generic metric theory may, in principle, predict waves with up to six different polarizations. This analysis is sensitive to continuous signals of scalar, vector, or tensor polarizations, and does not rely on any specific theory of gravity. After searching data from the first observation run of the advanced LIGO detectors for signals at twice the rotational frequency of 200 known pulsars, we find no evidence of gravitational waves of any polarization. We report the first upper limits for scalar and vector strains, finding values comparable in magnitude to previously published limits for tensor strain. Our results may be translated into constraints on specific alternative theories of gravity.", "date": "2018-01-19", "date_type": "published", "publication": "Physical Review Letters", "volume": "120", "number": "3", "publisher": "American Physical Society", "pagerange": "Art. No. 031104", "id_number": "CaltechAUTHORS:20180123-105038585", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180123-105038585", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia i Competitivitat" }, { "agency": "Conselleria d'Educaci\u00f3, Cultura i Universitats of the Govern de les Illes Balears" }, { "agency": "National Science Centre (Poland)" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Science and Engineering Research Council Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia, Inova\u00e7\u00e3o e Comunica\u00e7\u00e3o" }, { "agency": "Funda\u00e7ao de Amparo \u00e0 Pesquisa do Estado de S\u00e3o Paulo (FAPESP)" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1700009", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "Astronomy-Department" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevLett.120.031104", "primary_object": { "basename": "PhysRevLett.120.031104.pdf", "url": "https://authors.library.caltech.edu/records/dz3bq-zaf59/files/PhysRevLett.120.031104.pdf" }, "related_objects": [ { "basename": "cwpols_o1_tables.pdf", "url": "https://authors.library.caltech.edu/records/dz3bq-zaf59/files/cwpols_o1_tables.pdf" }, { "basename": "1709.09203.pdf", "url": "https://authors.library.caltech.edu/records/dz3bq-zaf59/files/1709.09203.pdf" } ], "resource_type": "article", "pub_year": "2018", "author_list": "Abbott, B. 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E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Blackman-J", "name": { "family": "Blackman", "given": "J." }, "orcid": "0000-0002-7113-0289" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Ma-Yiqiu", "name": { "family": "Ma", "given": "Y." }, "orcid": "0000-0001-7192-4874" }, { "id": "Pang-Belinda-Heyun", "name": { "family": "Pang", "given": "B." }, "orcid": "0000-0002-5697-2162" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Varma-V", "name": { "family": "Varma", "given": "V." }, "orcid": "0000-0002-9994-1761" } ] }, "title": "First low-frequency Einstein@Home all-sky search for continuous gravitational waves in Advanced LIGO data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2017 Published by the American Physical Society. Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. \n\nReceived 29 June 2017; revised manuscript received 14 September 2017; published 8 December 2017. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Econom\u00eda y Competitividad, the Vicepresid\u00e8ncia i Conselleria d'Innovaci\u00f3, Recerca i Turisme and the Conselleria d'Educaci\u00f3 i Universitat del Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR), Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS and the State of Niedersachsen/Germany for provision of computational resources. The authors also gratefully acknowledge the support of the many thousands of Einstein@Home volunteers, without whom this search would not have been possible. \n\nThis document has been assigned LIGO Laboratory document No. LIGO-P1700127.\n\nPublished - PhysRevD.96.122004.pdf
Submitted - 1707.02669.pdf
", "abstract": "We report results of a deep all-sky search for periodic gravitational waves from isolated neutron stars in data from the first Advanced LIGO observing run. This search investigates the low frequency range of Advanced LIGO data, between 20 and 100 Hz, much of which was not explored in initial LIGO. The search was made possible by the computing power provided by the volunteers of the Einstein@Home project. We find no significant signal candidate and set the most stringent upper limits to date on the amplitude of gravitational wave signals from the target population, corresponding to a sensitivity depth of 48.7\u2009\u2009[1/\u221aHz]. At the frequency of best strain sensitivity, near 100 Hz, we set 90% confidence upper limits of 1.8\u00d710^(\u221225). At the low end of our frequency range, 20 Hz, we achieve upper limits of 3.9\u00d710^(\u221224). At 55 Hz we can exclude sources with ellipticities greater than 10^(\u22125) within 100 pc of Earth with fiducial value of the principal moment of inertia of 10^(38)\u2009\u2009kg\u2009m^2.", "date": "2017-12-15", "date_type": "published", "publication": "Physical Review D", "volume": "96", "number": "12", "publisher": "American Physical Society", "pagerange": "Art. No. 122004", "id_number": "CaltechAUTHORS:20171213-083832918", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20171213-083832918", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Vicepresid\u00e8ncia i Conselleria d'Innovaci\u00f3, Recerca i Turisme" }, { "agency": "Conselleria d'Educaci\u00f3 i Universitat del Govern de les Illes Balears" }, { "agency": "National Science Centre (Poland)" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Science and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia, Inova\u00e7\u00e3o e Comunica\u00e7\u00e3o (MCTIC)" }, { "agency": "International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR)" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1700127", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "Astronomy-Department" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.96.122004", "primary_object": { "basename": "1707.02669.pdf", "url": "https://authors.library.caltech.edu/records/g3wxt-cq719/files/1707.02669.pdf" }, "related_objects": [ { "basename": "PhysRevD.96.122004.pdf", "url": "https://authors.library.caltech.edu/records/g3wxt-cq719/files/PhysRevD.96.122004.pdf" } ], "resource_type": "article", "pub_year": "2017", "author_list": "Abbott, B. 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C." } }, { "id": "Xiao-S", "name": { "family": "Xiao", "given": "S." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Barkett-K", "name": { "family": "Barkett", "given": "K." } }, { "id": "Blackman-J", "name": { "family": "Blackman", "given": "J." }, "orcid": "0000-0002-7113-0289" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Ma-Yiqiu", "name": { "family": "Ma", "given": "Y." }, "orcid": "0000-0001-7192-4874" }, { "id": "Pang-Belinda-Heyun", "name": { "family": "Pang", "given": "B." }, "orcid": "0000-0002-5697-2162" }, { "id": "Scheel-M-A", "name": { "family": "Scheel", "given": "M." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Varma-V", "name": { "family": "Varma", "given": "V." }, "orcid": "0000-0002-9994-1761" } ] }, "title": "GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2017 Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license.\n\nReceived 26 September 2017. Published 16 Oct 2017.\n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation (NSF) for the\nconstruction and operation of the LIGO Laboratory and\nAdvanced LIGO as well as the Science and Technology\nFacilities Council (STFC) of the United Kingdom, the Max-\nPlanck-Society (MPS), and the State of Niedersachsen,\nGermany for support of the construction of Advanced\nLIGO and construction and operation of the GEO600\ndetector. Additional support for Advanced LIGO was provided\nby the Australian Research Council. The authors\ngratefully acknowledge the Italian Istituto Nazionale di\nFisica Nucleare (INFN), the French Centre National de la\nRecherche Scientifique (CNRS), and the Foundation for\nFundamental Research on Matter supported by the\nNetherlands Organisation for Scientific Research, for the\nconstruction and operation of the Virgo detector and\nthe creation and support of the EGO consortium. The\nauthors also gratefully acknowledge research support from\nthese agencies as well as by the Council of Scientific and\nIndustrial Research of India, the Department of Science\nand Technology, India, the Science & Engineering\nResearch Board (SERB), India, the Ministry of Human\nResource Development, India, the Spanish Agencia\nEstatal de Investigaci\u00f3n, the Vicepresid\u00e8ncia i Conselleria\nd'Innovaci\u00f3, Recerca i Turisme and the Conselleria\nd'Educaci\u00f3 i Universitat del Govern de les Illes Balears,\nthe Conselleria d'Educaci\u00f3, Investigaci\u00f3, Cultura i Esport de\nla Generalitat Valenciana, the National Science Centre of\nPoland, the Swiss National Science Foundation (SNSF), the\nRussian Foundation for Basic Research, the Russian Science\nFoundation, the European Commission, the European\nRegional Development Funds (ERDF), the Royal Society,\nthe Scottish Funding Council, the Scottish Universities\nPhysics Alliance, the Hungarian Scientific Research Fund\n(OTKA), the Lyon Institute of Origins (LIO), the National\nResearch, Development and Innovation Office Hungary\n(NKFI), the National Research Foundation of Korea,\nIndustry Canada and the Province of Ontario through the\nMinistry of Economic Development and Innovation, the\nNatural Science and Engineering Research Council Canada,\nthe Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, Innovations, and\nCommunications, the International Center for Theoretical\nPhysics South American Institute for Fundamental Research\n(ICTP-SAIFR), the Research Grants Council of Hong Kong,\nthe National Natural Science Foundation of China (NSFC),\nthe Leverhulme Trust, the Research Corporation, the\nMinistry of Science and Technology (MOST), Taiwan and\nthe Kavli Foundation. The authors gratefully acknowledge\nthe support of the NSF, STFC, MPS, INFN, CNRS and the\nState of Niedersachsen, Germany for provision of computational\nresources. This research has made use of the\nNASA/IPAC Extragalactic Database (NED) which is operated\nby the Jet Propulsion Laboratory, California Institute of\nTechnology, under contract with the National Aeronautics\nand Space Administration.\n\nPublished - PhysRevLett.119.161101
", "abstract": "On August 17, 2017 at 12\u223641:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0\u00d710^4\u2009\u2009years. We infer the component masses of the binary to be between 0.86 and 2.26\u2009\u2009M\u2299, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17\u20131.60\u2009\u2009M\u2299, with the total mass of the system 2.74^(+0.04)_(\u22120.01)M\u2299. The source was localized within a sky region of 28\u2009\u2009deg^2(90% probability) and had a luminosity distance of 40^(+8)_(\u221214)\u2009\u2009Mpc, the closest and most precisely localized gravitational-wave signal yet. The association with the \u03b3-ray burst GRB 170817A, detected by Fermi-GBM 1.7 s after the coalescence, corroborates the hypothesis of a neutron star merger and provides the first direct evidence of a link between these mergers and short \u03b3-ray bursts. Subsequent identification of transient counterparts across the electromagnetic spectrum in the same location further supports the interpretation of this event as a neutron star merger. This unprecedented joint gravitational and electromagnetic observation provides insight into astrophysics, dense matter, gravitation, and cosmology.", "date": "2017-10-20", "date_type": "published", "publication": "Physical Review Letters", "volume": "119", "number": "16", "publisher": "American Physical Society", "pagerange": "Art No. 161101", "id_number": "CaltechAUTHORS:20171016-090538618", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20171016-090538618", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Agencia Estatal de Investigaci\u00f3n" }, { "agency": "Vicepresid\u00e8ncia i Conselleria d'Innovaci\u00f3, Recerca i Turisme" }, { "agency": "Conselleria d'Educaci\u00f3 i Universitat del Govern de les Illes Balears" }, { "agency": "Conselleria d'Educaci\u00f3, Investigaci\u00f3, Cultura i Esport de la Generalitat Valenciana" }, { "agency": "National Science Centre (Poland)" }, { "agency": "Swiss National Science Foundation (SNSF)" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Russian Science Foundation" }, { "agency": "European Commission" }, { "agency": "European Regional Development Fund (ERDF)" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research, Development and Innovation Office (Hungary)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Science and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia, Inova\u00e7\u00e3o e Comunica\u00e7\u00e3o" }, { "agency": "International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR)" }, { "agency": "Research Grants Council of Hong Kong" }, { "agency": "National Natural Science Foundation of China" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" }, { "agency": "NASA/JPL/Caltech" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "Astronomy-Department" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevLett.119.161101", "primary_object": { "basename": "PhysRevLett.119.161101", "url": "https://authors.library.caltech.edu/records/10k3g-h8z59/files/PhysRevLett.119.161101" }, "resource_type": "article", "pub_year": "2017", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/mwmdd-w8157", "eprint_id": 81361, "eprint_status": "archive", "datestamp": "2023-08-19 05:08:25", "lastmod": "2023-10-17 19:47:36", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ananyeva-A", "name": { "family": "Ananyeva", "given": "A." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Appert-S", "name": { "family": "Appert", "given": "S." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Berger-B-K", "name": { "family": "Berger", "given": "B. K." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Brunett-S", "name": { "family": "Brunett", "given": "S." } }, { "id": "Cahillane-C", "name": { "family": "Cahillane", "given": "C." } }, { "id": "Callister-T-A", "name": { "family": "Callister", "given": "T. A." }, "orcid": "0000-0001-9892-177X" }, { "id": "Cepeda-C-B", "name": { "family": "Cepeda", "given": "C. B." } }, { "id": "Couvares-P", "name": { "family": "Couvares", "given": "P." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Eichholz-J", "name": { "family": "Eichholz", "given": "J." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Feicht-J", "name": { "family": "Feicht", "given": "J." } }, { "id": "Fries-E-M", "name": { "family": "Fries", "given": "E. M." } }, { "id": "Gossan-S-E", "name": { "family": "Gossan", "given": "S. E." }, "orcid": "0000-0002-8138-9198" }, { "id": "Gushwa-K-E", "name": { "family": "Gushwa", "given": "K. E." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hall-E-D", "name": { "family": "Hall", "given": "E. D." }, "orcid": "0000-0001-9018-666X" }, { "id": "Heptonstall-A-W", "name": { "family": "Heptonstall", "given": "A. W." } }, { "id": "Isi-M", "name": { "family": "Isi", "given": "M." }, "orcid": "0000-0001-8830-8672" }, { "id": "Kanner-J-B", "name": { "family": "Kanner", "given": "J. B." }, "orcid": "0000-0001-8115-0577" }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Korth-W-Z", "name": { "family": "Korth", "given": "W. Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D. B." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Massinger-T-J", "name": { "family": "Massinger", "given": "T. J." }, "orcid": "0000-0002-3429-5025" }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "McIver-J", "name": { "family": "McIver", "given": "J." }, "orcid": "0000-0003-0316-1355" }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Perreca-A", "name": { "family": "Perreca", "given": "A." } }, { "id": "Quintero-E-A", "name": { "family": "Quintero", "given": "E. A." } }, { "id": "Reitze-D-H", "name": { "family": "Reitze", "given": "D. H." } }, { "id": "Rollins-J-G", "name": { "family": "Rollins", "given": "J. G." } }, { "id": "Sachdev-S", "name": { "family": "Sachdev", "given": "S." }, "orcid": "0000-0002-2432-7070" }, { "id": "Sanchez-E-J", "name": { "family": "Sanchez", "given": "E. J." } }, { "id": "Schmidt-P", "name": { "family": "Schmidt", "given": "P." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-R-J-E", "name": { "family": "Smith", "given": "R. J. E." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Tso-Rhondale", "name": { "family": "Tso", "given": "R." }, "orcid": "0000-0003-4464-0117" }, { "id": "Urban-A-L", "name": { "family": "Urban", "given": "A. L." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Venugopalan-G", "name": { "family": "Venugopalan", "given": "G." } }, { "id": "Wade-A-R", "name": { "family": "Wade", "given": "A. R." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Blackman-J", "name": { "family": "Blackman", "given": "J." }, "orcid": "0000-0002-7113-0289" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Ma-Yiqiu", "name": { "family": "Ma", "given": "Y." }, "orcid": "0000-0001-7192-4874" }, { "id": "Pang-Belinda-Heyun", "name": { "family": "Pang", "given": "B." }, "orcid": "0000-0002-5697-2162" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Varma-V", "name": { "family": "Varma", "given": "V." }, "orcid": "0000-0002-9994-1761" } ] }, "title": "All-sky search for periodic gravitational waves in the O1 LIGO data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2017 American Physical Society. \n\nReceived 10 July 2017; published 12 September 2017. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India; Department of Science and Technology, India; Science & Engineering Research Board (SERB), India; Ministry of Human Resource Development, India; the Spanish Ministerio de Econom\u00eda y Competitividad; the Vicepresid\u00e8ncia i Conselleria d'Innovaci\u00f3; Recerca i Turisme and the Conselleria d'Educaci\u00f3 i Universitat del Govern de les Illes Balears; the National Science Centre of Poland; the European Commission; the Royal Society; the Scottish Funding Council; the Scottish Universities Physics Alliance; the Hungarian Scientific Research Fund (OTKA); the Lyon Institute of Origins (LIO); the National Research Foundation of Korea; Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation; the Natural Science and Engineering Research Council Canada; Canadian Institute for Advanced Research; the Brazilian Ministry of Science, Technology, and Innovation; International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR); Russian Foundation for Basic Research; the Leverhulme Trust; the Research Corporation,; Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, PL-Grid and the State of Niedersachsen/Germany for provision of computational resources. This document has been assigned LIGO Laboratory document No. LIGO-P1700052-v18.\n\nPublished - PhysRevD.96.062002.pdf
Submitted - 1707.02667.pdf
", "abstract": "We report on an all-sky search for periodic gravitational waves in the frequency band 20\u2013475 Hz and with a frequency time derivative in the range of [\u22121.0,+0.1] \u00d7 10^(\u22128)\u2009Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our galaxy. This search uses the data from Advanced LIGO's first observational run, O1. No periodic gravitational wave signals were observed, and upper limits were placed on their strengths. The lowest upper limits on worst-case (linearly polarized) strain amplitude h_0 are \u223c4 \u00d7 10^(\u221225) near 170 Hz. For a circularly polarized source (most favorable orientation), the smallest upper limits obtained are \u223c1.5 \u00d7 10^(\u221225). These upper limits refer to all sky locations and the entire range of frequency derivative values. For a population-averaged ensemble of sky locations and stellar orientations, the lowest upper limits obtained for the strain amplitude are ~2.5 \u00d7 10^(\u221225).", "date": "2017-09-15", "date_type": "published", "publication": "Physical Review D", "volume": "96", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 062002", "id_number": "CaltechAUTHORS:20170912-124106618", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170912-124106618", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society (MPS)" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "French Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Vicepresid\u00e8ncia i Conselleria d'Innovaci\u00f3, Recerca i Turisme" }, { "agency": "Conselleria d'Educaci\u00f3 i Universitat del Govern de les Illes Balears" }, { "agency": "National Science Centre (Poland)" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia, Inova\u00e7\u00e3o e Comunica\u00e7\u00e3o" }, { "agency": "International Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR)" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Taiwan Foundation" }, { "agency": "Kavli Foundation" }, { "agency": "NSF" }, { "agency": "PL-Grid" } ] }, "other_numbering_system": { "items": [ { "id": "P-1700052-v.18", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "Astronomy-Department" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.96.062002", "primary_object": { "basename": "1707.02667.pdf", "url": "https://authors.library.caltech.edu/records/mwmdd-w8157/files/1707.02667.pdf" }, "related_objects": [ { "basename": "PhysRevD.96.062002.pdf", "url": "https://authors.library.caltech.edu/records/mwmdd-w8157/files/PhysRevD.96.062002.pdf" } ], "resource_type": "article", "pub_year": "2017", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/f4q3f-wa154", "eprint_id": 78518, "eprint_status": "archive", "datestamp": "2023-08-19 02:55:37", "lastmod": "2023-10-26 00:10:06", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" }, { "id": "van-Haasteren-R", "name": { "family": "van Haasteren", "given": "Rutger" }, "orcid": "0000-0002-6428-2620" } ] }, "title": "Taming outliers in pulsar-timing data sets with hierarchical likelihoods and Hamiltonian sampling", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves \u2013 methods: data analysis \u2013 pulsars: general", "note": "\u00a9 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. \n\nAccepted 2017 January 10. Received 2016 December 17; in original form 2016 September 19. Published: 20 January 2017. \n\nWe thank B. Bassett, E. Cameron, N. Cornish, C. Cutler, J. Ellis, J. Lazio, C. Mingarelli, D. Nice, S. Taylor and the anonymous MNRAS referee for useful comments. MV was supported by the Jet Propulsion Laboratory RTD programme. RvH was supported by NASA Einstein Fellowship grant PF3-140116. This research was supported in part by National Science Foundation Physics Frontier Center award no. 1430284, and by grant PHYS-1066293 and the hospitality of the Aspen Center for Physics. This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract to the National Aeronautics and Space Administration. Copyright 2016 California Institute of Technology. Government sponsorship acknowledged.\n\nPublished - stx069.pdf
Submitted - 1609.02144.pdf
", "abstract": "Pulsar-timing data sets have been analysed with great success using probabilistic treatments based on Gaussian distributions, with applications ranging from studies of neutron-star structure to tests of general relativity and searches for nanosecond gravitational waves. As for other applications of Gaussian distributions, outliers in timing measurements pose a significant challenge to statistical inference, since they can bias the estimation of timing and noise parameters, and affect reported parameter uncertainties. We describe and demonstrate a practical end-to-end approach to perform Bayesian inference of timing and noise parameters robustly in the presence of outliers, and to identify these probabilistically. The method is fully consistent (i.e. outlier-ness probabilities vary in tune with the posterior distributions of the timing and noise parameters), and it relies on the efficient sampling of the hierarchical form of the pulsar-timing likelihood. Such sampling has recently become possible with a 'no-U-turn' Hamiltonian sampler coupled to a highly customized reparametrization of the likelihood; this code is described elsewhere, but it is already available online. We recommend our method as a standard step in the preparation of pulsar-timing-array data sets: even if statistical inference is not affected, follow-up studies of outlier candidates can reveal unseen problems in radio observations and timing measurements; furthermore, confidence in the results of gravitational-wave searches will only benefit from stringent statistical evidence that data sets are clean and outlier-free.", "date": "2017-05", "date_type": "published", "publication": "Monthly Notices of the Royal Astronomical Society", "volume": "466", "number": "4", "publisher": "Royal Astronomical Society", "pagerange": "4954-4959", "id_number": "CaltechAUTHORS:20170623-123731334", "issn": "0035-8711", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170623-123731334", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NASA Einstein Fellowship", "grant_number": "PF3-140116" }, { "agency": "NSF", "grant_number": "1430284" }, { "agency": "NSF", "grant_number": "PHYS-1066293" }, { "agency": "NASA/JPL/Caltech" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1093/mnras/stx069", "primary_object": { "basename": "1609.02144.pdf", "url": "https://authors.library.caltech.edu/records/f4q3f-wa154/files/1609.02144.pdf" }, "related_objects": [ { "basename": "stx069.pdf", "url": "https://authors.library.caltech.edu/records/f4q3f-wa154/files/stx069.pdf" } ], "resource_type": "article", "pub_year": "2017", "author_list": "Vallisneri, Michele and van Haasteren, Rutger" }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/10759-thc24", "eprint_id": 71003, "eprint_status": "archive", "datestamp": "2023-08-22 19:16:39", "lastmod": "2023-10-23 20:11:08", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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J." } }, { "id": "Schmidt-P", "name": { "family": "Schmidt", "given": "P." } }, { "id": "Shao-Z", "name": { "family": "Shao", "given": "Z." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-N-D", "name": { "family": "Smith", "given": "N. D." } }, { "id": "Smith-R-J-E", "name": { "family": "Smith", "given": "R. J. E." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; stars: massive", "note": "\u00a9 2016 American Astronomical Society. \n\nReceived 2016 February 12. Accepted 2016 September 19. Published 2016 November 30. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3, Cultura i Universitats of the Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, Ministry of Science and Technology (MOST), Taiwan and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS and the State of Niedersachsen/Germany for provision of computational resources. This article has been assigned the document number LIGO-P1500217.\n\nPublished - Abbott_2016_ApJL_833_L1.pdf
Submitted - 1602.03842v3.pdf
Supplemental Material - 1602.03842v2-Supplement.pdf
", "abstract": "A transient gravitational-wave signal, GW150914, was identified in the twin Advanced LIGO detectors on September 14, 2015 at 09:50:45 UTC. To assess the implications of this discovery, the detectors remained in operation with unchanged configurations over a period of 39 d around the time of the signal. At the detection statistic threshold corresponding to that observed for GW150914, our search of the 16 days of simultaneous two-detector observational data is estimated to have a false alarm rate (FAR) of < 4.9 \u00d7 10^(\u22126) yr^(\u22121), yielding a p-value for GW150914 of < 2 \u00d7 10^(\u22127). Parameter estimation followup on this trigger identifies its source as a binary black hole (BBH) merger with component masses (m_1, m_2) = (36^(+5)_(\u22124), 29^(+4)_(\u22124)) M_\u2299 at redshift z = 0.09^(+0.03)_(\u22120.04) (median and 90\\% credible range). Here we report on the constraints these observations place on the rate of BBH coalescences. Considering only GW150914, assuming that all BBHs in the Universe have the same masses and spins as this event, imposing a search FAR threshold of 1 per 100 years, and assuming that the BBH merger rate is constant in the comoving frame, we infer a 90% credible range of merger rates between 2--53 Gpc^(\u22123) yr^(\u22121) (comoving frame). Incorporating all search triggers that pass a much lower threshold while accounting for the uncertainty in the astrophysical origin of each trigger, we estimate a higher rate, ranging from 13--600 Gpc^(\u22123) yr^(\u22121) depending on assumptions about the BBH mass distribution. All together, our various rate estimates fall in the conservative range 2--600 Gpc^(\u22123) yr^(\u22121).", "date": "2016-12-10", "date_type": "published", "publication": "Astrophysical Journal Letters", "volume": "833", "number": "1", "publisher": "American Astronomical Society", "pagerange": "Art. No. L1", "id_number": "CaltechAUTHORS:20161011-161919040", "issn": "2041-8205", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20161011-161919040", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society (MPS)" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3" }, { "agency": "Cultura i Universitats of the Govern de les Illes Balears" }, { "agency": "National Science Centre (Poland)" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Research and Innovation" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia e Inova\u00e7\u00e3o" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1500217", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "VIRGO Collaboration" ] }, "doi": "10.3847/2041-8205/833/1/L1", "primary_object": { "basename": "1602.03842v2-Supplement.pdf", "url": "https://authors.library.caltech.edu/records/10759-thc24/files/1602.03842v2-Supplement.pdf" }, "related_objects": [ { "basename": "1602.03842v3.pdf", "url": "https://authors.library.caltech.edu/records/10759-thc24/files/1602.03842v3.pdf" }, { "basename": "Abbott_2016_ApJL_833_L1.pdf", "url": "https://authors.library.caltech.edu/records/10759-thc24/files/Abbott_2016_ApJL_833_L1.pdf" } ], "resource_type": "article", "pub_year": "2016", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/nsy31-51015", "eprint_id": 71724, "eprint_status": "archive", "datestamp": "2023-08-22 19:12:09", "lastmod": "2023-10-23 17:01:13", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abernathy-M-R", "name": { "family": "Abernathy", "given": "M. R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. 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I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Engels-W", "name": { "family": "Engels", "given": "W." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; stars: black holes", "note": "\u00a9 2016 American Astronomical Society. \n\nReceived 2016 May 27. Accepted 2016 September 22. Published 2016 November 30. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO, as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector, and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well: the Council of Scientific and Industrial Research of India, the Department of Science and Technology, India, the Science & Engineering Research Board (SERB), India, the Ministry of Human Resource Development, India, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3 Cultura i Universitats of the Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, the Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, the Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, the Ministry of Science and Technology (MOST), Taiwan, and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, and the State of Niedersachsen/Germany for the provision of computational resources. This article has been assigned the document number LIGO-P1500217.\n\nPublished - Abbott_2016_ApJS_227_14.pdf
Submitted - 1606.03939v2.pdf
", "abstract": "This article provides supplemental information for a Letter reporting the rate of (BBH) coalescences inferred from 16 days of coincident Advanced LIGO observations surrounding the transient (GW) signal GW150914. In that work we reported various rate estimates whose 90% confidence intervals fell in the range 2\u2013600 Gpc^(\u22123) yr^(\u22121). Here we give details on our method and computations, including information about our search pipelines, a derivation of our likelihood function for the analysis, a description of the astrophysical search trigger distribution expected from merging BBHs, details on our computational methods, a description of the effects and our model for calibration uncertainty, and an analytic method for estimating our detector sensitivity, which is calibrated to our measurements.", "date": "2016-12", "date_type": "published", "publication": "Astrophysical Journal Supplement Series", "volume": "227", "number": "2", "publisher": "American Astronomical Society", "pagerange": "Art. No. 14", "id_number": "CaltechAUTHORS:20161103-144139033", "issn": "0067-0049", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20161103-144139033", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia i Competitivitat" }, { "agency": "Conselleria d'Educaci\u03cc, Cultura i Universitats of the Govern de les Illes Balears" }, { "agency": "National Science Centre (Poland)" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Science and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia e Inova\u00e7\u00e3o" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ontario Ministry of Economic Development and Innovation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1500217", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.3847/0067-0049/227/2/14", "primary_object": { "basename": "1606.03939v2.pdf", "url": "https://authors.library.caltech.edu/records/nsy31-51015/files/1606.03939v2.pdf" }, "related_objects": [ { "basename": "Abbott_2016_ApJS_227_14.pdf", "url": "https://authors.library.caltech.edu/records/nsy31-51015/files/Abbott_2016_ApJS_227_14.pdf" } ], "resource_type": "article", "pub_year": "2016", "author_list": "Abbott, B. P.; Abernathy, M. R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/p2eb7-xnd54", "eprint_id": 71557, "eprint_status": "archive", "datestamp": "2023-08-20 14:02:51", "lastmod": "2023-10-23 15:54:32", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Berger-B-K", "name": { "family": "Berger", "given": "B. K." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Brunett-S", "name": { "family": "Brunett", "given": "S." } }, { "id": "Cahillane-C", "name": { "family": "Cahillane", "given": "C." } }, { "id": "Callister-T-A", "name": { "family": "Callister", "given": "T." }, "orcid": "0000-0001-9892-177X" }, { "id": "Cepeda-C-B", "name": { "family": "Cepeda", "given": "C. B." } }, { "id": "Couvares-P", "name": { "family": "Couvares", "given": "P." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Eichholz-J", "name": { "family": "Eichholz", "given": "J." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Gossan-S-E", "name": { "family": "Gossan", "given": "S. E." }, "orcid": "0000-0002-8138-9198" }, { "id": "Gushwa-K-E", "name": { "family": "Gushwa", "given": "K. E." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hall-E-D", "name": { "family": "Hall", "given": "E. D." }, "orcid": "0000-0001-9018-666X" }, { "id": "Heptonstall-A-W", "name": { "family": "Heptonstall", "given": "A. W." } }, { "id": "Isi-M", "name": { "family": "Isi", "given": "M." }, "orcid": "0000-0001-8830-8672" }, { "id": "Kanner-J-B", "name": { "family": "Kanner", "given": "J. B." }, "orcid": "0000-0001-8115-0577" }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Korth-W-Z", "name": { "family": "Korth", "given": "W. Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D. B." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lewis-J-B", "name": { "family": "Lewis", "given": "J. B." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "McIver-J", "name": { "family": "McIver", "given": "J." }, "orcid": "0000-0003-0316-1355" }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Perreca-A", "name": { "family": "Perreca", "given": "A." } }, { "id": "Price-L-R", "name": { "family": "Price", "given": "L. R." } }, { "id": "Quintero-E-A", "name": { "family": "Quintero", "given": "E. A." } }, { "id": "Reitze-D-H", "name": { "family": "Reitze", "given": "D. H." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Rollins-J-G", "name": { "family": "Rollins", "given": "J. G." } }, { "id": "Sachdev-S", "name": { "family": "Sachdev", "given": "S." }, "orcid": "0000-0002-2432-7070" }, { "id": "Sanchez-E-J", "name": { "family": "Sanchez", "given": "E. J." } }, { "id": "Schmidt-P", "name": { "family": "Schmidt", "given": "P." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-N-D", "name": { "family": "Smith", "given": "N. D." } }, { "id": "Smith-R-J-E", "name": { "family": "Smith", "given": "R. J. E." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Engels-W", "name": { "family": "Engels", "given": "W." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Binary Black Hole Mergers in the First Advanced LIGO Observing Run", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2016 Published by the American Physical Society under the terms of the Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. \n\nReceived 24 June 2016; revised manuscript received 8 August 2016; published 21 October 2016. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO, as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies, as well as by the Council of Scientific and Industrial Research of India; Department of Science and Technology, India; Science & Engineering Research Board (SERB), India; Ministry of Human Resource Development, India; the Spanish Ministerio de Econom\u00eda y Competitividad; the Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3; Cultura i Universitats of the Govern de les Illes Balears; the National Science Centre of Poland; the European Commission; the Royal Society; the Scottish Funding Council; the Scottish Universities Physics Alliance; the Hungarian Scientific Research Fund (OTKA); the Lyon Institute of Origins (LIO); the National Research Foundation of Korea; Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation; the Natural Science and Engineering Research Council Canada; Canadian Institute for Advanced Research; the Brazilian Ministry of Science, Technology, and Innovation; Funda\u0107\u00e3o de Amparo \u00e0 Pesquisa do Estado de S\u00e3o Paulo (FAPESP); Russian Foundation for Basic Research; the Leverhulme Trust, the Research Corporation; Ministry of Science and Technology (MOST), Taiwan; and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, and the State of Niedersachsen/Germany for provision of computational resources.\n\nPublished - PhysRevX.6.041015.pdf
Submitted - 1606.04856v2.pdf
", "abstract": "The first observational run of the Advanced LIGO detectors, from September 12, 2015 to January 19, 2016, saw the first detections of gravitational waves from binary black hole mergers. In this paper, we present full results from a search for binary black hole merger signals with total masses up to 100M\u2299 and detailed implications from our observations of these systems. Our search, based on general-relativistic models of gravitational-wave signals from binary black hole systems, unambiguously identified two signals, GW150914 and GW151226, with a significance of greater than 5\u03c3 over the observing period. It also identified a third possible signal, LVT151012, with substantially lower significance and with an 87% probability of being of astrophysical origin. We provide detailed estimates of the parameters of the observed systems. Both GW150914 and GW151226 provide an unprecedented opportunity to study the two-body motion of a compact-object binary in the large velocity, highly nonlinear regime. We do not observe any deviations from general relativity, and we place improved empirical bounds on several high-order post-Newtonian coefficients. From our observations, we infer stellar-mass binary black hole merger rates lying in the range 9\u2013240\u2009Gpc^(\u22123) \u2009yr^(\u22121). These observations are beginning to inform astrophysical predictions of binary black hole formation rates and indicate that future observing runs of the Advanced detector network will yield many more gravitational-wave detections.", "date": "2016-10", "date_type": "published", "publication": "Physical Review X", "volume": "6", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 041015", "id_number": "CaltechAUTHORS:20161027-140916426", "issn": "2160-3308", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20161027-140916426", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3" }, { "agency": "Cultura i Universitats of the Govern de les Illes Balears" }, { "agency": "National Science Centre (Poland)" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Research and Innovation" }, { "agency": "Natural Science and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia e Inova\u00e7\u00e3o" }, { "agency": "Funda\u0107\u00e3o de Amparo \u00e0 Pesquisa do Estado de S\u00e3o Paulo (FAPESP)" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevX.6.041015", "primary_object": { "basename": "PhysRevX.6.041015.pdf", "url": "https://authors.library.caltech.edu/records/p2eb7-xnd54/files/PhysRevX.6.041015.pdf" }, "related_objects": [ { "basename": "1606.04856v2.pdf", "url": "https://authors.library.caltech.edu/records/p2eb7-xnd54/files/1606.04856v2.pdf" } ], "resource_type": "article", "pub_year": "2016", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/2meeg-04d09", "eprint_id": 71440, "eprint_status": "archive", "datestamp": "2023-08-20 14:02:44", "lastmod": "2023-10-23 15:46:15", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. 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C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Gossan-S-E", "name": { "family": "Gossan", "given": "S. E." }, "orcid": "0000-0002-8138-9198" }, { "id": "Gushwa-K-E", "name": { "family": "Gushwa", "given": "K. E." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hall-E-D", "name": { "family": "Hall", "given": "E. D." }, "orcid": "0000-0001-9018-666X" }, { "id": "Heptonstall-A-W", "name": { "family": "Heptonstall", "given": "A. W." } }, { "id": "Isi-M", "name": { "family": "Isi", "given": "M." }, "orcid": "0000-0001-8830-8672" }, { "id": "Kanner-J-B", "name": { "family": "Kanner", "given": "J. B." }, "orcid": "0000-0001-8115-0577" }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Korth-W-Z", "name": { "family": "Korth", "given": "W. Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D. B." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lewis-J-B", "name": { "family": "Lewis", "given": "J. B." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "McIver-J", "name": { "family": "McIver", "given": "J." }, "orcid": "0000-0003-0316-1355" }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Perreca-A", "name": { "family": "Perreca", "given": "A." } }, { "id": "Price-L-R", "name": { "family": "Price", "given": "L. R." } }, { "id": "Quintero-E-A", "name": { "family": "Quintero", "given": "E. A." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Rollins-J-G", "name": { "family": "Rollins", "given": "J. G." } }, { "id": "Sachdev-S", "name": { "family": "Sachdev", "given": "S." }, "orcid": "0000-0002-2432-7070" }, { "id": "Sanchez-E-J", "name": { "family": "Sanchez", "given": "E. J." } }, { "id": "Schmidt-P", "name": { "family": "Schmidt", "given": "P." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-N-D", "name": { "family": "Smith", "given": "N. D." } }, { "id": "Smith-R-J-E", "name": { "family": "Smith", "given": "R. J. E." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Engels-W", "name": { "family": "Engels", "given": "W." } }, { "id": "Hemberger-D-A", "name": { "family": "Hemberger", "given": "D." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Scheel-M-A", "name": { "family": "Scheel", "given": "M." } }, { "id": "Szil\u00e1gyi-B", "name": { "family": "Szil\u00e1gyi", "given": "B." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Teukolsky-S-A", "name": { "family": "Teukolsky", "given": "S." }, "orcid": "0000-0001-9765-4526" } ] }, "title": "Improved analysis of GW150914 using a fully spin-precessing waveform model", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2016 Published by the American Physical Society under the terms of the Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI.\n\n\nReceived 4 June 2016; revised manuscript received 30 July 2016; published 21 October 2016.\n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO, as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies, as well as by the Council of Scientific and Industrial Research of India; Department of Science and Technology, India; Science & Engineering Research Board (SERB), India; Ministry of Human Resource Development, India; the Spanish Ministerio de Econom\u00eda y Competitividad; the Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3; Cultura i Universitats of the Govern de les Illes Balears; the National Science Centre of Poland; the European Commission; the Royal Society; the Scottish Funding Council; the Scottish Universities Physics Alliance; the Hungarian Scientific Research Fund (OTKA); the Lyon Institute of Origins (LIO); the National Research Foundation of Korea; Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation; the Natural Science and Engineering Research Council Canada; Canadian Institute for Advanced Research; the Brazilian Ministry of Science, Technology, and Innovation; Russian Foundation for Basic Research; the Leverhulme Trust; the Research Corporation; Ministry of Science and Technology (MOST), Taiwan; and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, and the State of Niedersachsen/Germany for provision of computational resources.\n\nPublished - PhysRevX.6.041014.pdf
Submitted - 1606.01210v1.pdf
", "abstract": "This paper presents updated estimates of source parameters for GW150914, a binary black-hole coalescence event detected by the Laser Interferometer Gravitational-wave Observatory (LIGO) in 2015 [Abbott et al. Phys. Rev. Lett. 116, 061102 (2016).]. Abbott et al. [Phys. Rev. Lett. 116, 241102 (2016).] presented parameter estimation of the source using a 13-dimensional, phenomenological precessing-spin model (precessing IMRPhenom) and an 11-dimensional nonprecessing effective-one-body (EOB) model calibrated to numerical-relativity simulations, which forces spin alignment (nonprecessing EOBNR). Here, we present new results that include a 15-dimensional precessing-spin waveform model (precessing EOBNR) developed within the EOB formalism. We find good agreement with the parameters estimated previously [Abbott et al. Phys. Rev. Lett. 116, 241102 (2016).], and we quote updated component masses of 35^(+5)_(\u22123) M\u2299 and 30^(+3)_(\u22124) M\u2299 (where errors correspond to 90% symmetric credible intervals). We also present slightly tighter constraints on the dimensionless spin magnitudes of the two black holes, with a primary spin estimate <0.65 and a secondary spin estimate <0.75 at 90% probability. Abbott et al. [Phys. Rev. Lett. 116, 241102 (2016).] estimated the systematic parameter-extraction errors due to waveform-model uncertainty by combining the posterior probability densities of precessing IMRPhenom and nonprecessing EOBNR. Here, we find that the two precessing-spin models are in closer agreement, suggesting that these systematic errors are smaller than previously quoted.", "date": "2016-10", "date_type": "published", "publication": "Physical Review X", "volume": "6", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 041014", "id_number": "CaltechAUTHORS:20161025-090158516", "issn": "2160-3308", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20161025-090158516", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science & Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia i Competitivitat" }, { "agency": "Conselleria d'Educaci\u03cc, Cultura i Universitats of the Govern de les Illes Balears" }, { "agency": "National Science Centre (Poland)" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Science and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIFAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia e Inova\u00e7\u00e3o" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevX.6.041014", "primary_object": { "basename": "1606.01210v1.pdf", "url": "https://authors.library.caltech.edu/records/2meeg-04d09/files/1606.01210v1.pdf" }, "related_objects": [ { "basename": "PhysRevX.6.041014.pdf", "url": "https://authors.library.caltech.edu/records/2meeg-04d09/files/PhysRevX.6.041014.pdf" } ], "resource_type": "article", "pub_year": "2016", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/vy9wf-29q32", "eprint_id": 74492, "eprint_status": "archive", "datestamp": "2023-08-20 14:05:43", "lastmod": "2023-10-24 22:41:53", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Holst-M", "name": { "family": "Holst", "given": "Michael" } }, { "id": "Sarbach-O", "name": { "family": "Sarbach", "given": "Olivier" } }, { "id": "Tiglio-M", "name": { "family": "Tiglio", "given": "Manuel" } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "The emergence of gravitational wave science: 100 years of development of mathematical theory, detectors, numerical algorithms, and data analysis tools", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2016 American Mathematical Society. \n\nArticle electronically published on August 2, 2016. \n\nWe thank the reviewers as well as David Shoemaker, who read preliminary drafts, for their feedback and comments. This work was supported in part by NSF grants PHY-1500818, DMS/FRG-1262982, and DMS/CM-1217175 to the University of\nCalifornia at San Diego, by NSF grant PHY-1404569 to the California Institute of Technology, by CONACyT grant No. 271904, and by a CIC grant to Universidad Michoacana. Part of this research was performed at the Jet Propulsion Laboratory, under contract with the National Aeronautics and Space Administration.\n\nSubmitted - 1607.05251.pdf
", "abstract": "On September 14, 2015, the newly upgraded Laser Interferometer Gravitational-wave Observatory (LIGO) recorded a loud gravitational-wave (GW) signal, emitted a billion light-years away by a coalescing binary of two stellar-mass black holes. The detection was announced in February 2016, in time for the hundredth anniversary of Einstein's prediction of GWs within the theory of general relativity (GR). The signal represents the first direct detection of GWs, the first observation of a black-hole binary, and the first test of GR in its strong-field, high-velocity, nonlinear regime. In the remainder of its first observing run, LIGO observed two more signals from black-hole binaries, one moderately loud, another at the boundary of statistical significance. The detections mark the end of a decades-long quest and the beginning of GW astronomy: finally, we are able to probe the unseen, electromagnetically dark Universe by listening to it. In this article, we present a short historical overview of GW science: this young discipline combines GR, arguably the crowning achievement of classical physics, with record-setting, ultra-low-noise laser interferometry, and with some of the most powerful developments in the theory of differential geometry, partial differential equations, high-performance computation, numerical analysis, signal processing, statistical inference, and data science. Our emphasis is on the synergy between these disciplines and how mathematics, broadly understood, has historically played, and continues to play, a crucial role in the development of GW science. We focus on black holes, which are very pure mathematical solutions of Einstein's gravitational-field equations that are nevertheless realized in Nature and that provided the first observed signals.", "date": "2016-10", "date_type": "published", "publication": "Bulletin of the American Mathematical Society", "volume": "53", "number": "4", "publisher": "American Mathematical Society", "pagerange": "513-554", "id_number": "CaltechAUTHORS:20170223-100913579", "issn": "0273-0979", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170223-100913579", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "PHY-1500818" }, { "agency": "NSF", "grant_number": "DMS-1262982" }, { "agency": "NSF", "grant_number": "DMS-1217175" }, { "agency": "NSF", "grant_number": "PHY-1404569" }, { "agency": "Consejo Nacional de Ciencia y Tecnolog\u00eda (CONACYT)", "grant_number": "271904" }, { "agency": "Coordinaci\u00f3n de Investigaci\u00f3n Cient\u00edfica (CIC)" }, { "agency": "JPL/NASA" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "doi": "10.1090/bull/1544", "primary_object": { "basename": "1607.05251.pdf", "url": "https://authors.library.caltech.edu/records/vy9wf-29q32/files/1607.05251.pdf" }, "resource_type": "article", "pub_year": "2016", "author_list": "Holst, Michael; Sarbach, Olivier; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/qqfw7-0x416", "eprint_id": 67944, "eprint_status": "archive", "datestamp": "2023-09-15 05:27:11", "lastmod": "2023-10-23 21:17:35", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Engels-W", "name": { "family": "Engels", "given": "W." } }, { "id": "Schmidt-P", "name": { "family": "Schmidt", "given": "P." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Hemberger-D-A", "name": { "family": "Hemberger", "given": "D." } }, { "id": "Scheel-M-A", "name": { "family": "Scheel", "given": "M." } }, { "id": "Szil\u00e1gyi-B", "name": { "family": "Szil\u00e1gyi", "given": "B." } }, { "id": "Teukolsky-S-A", "name": { "family": "Teukolsky", "given": "S." }, "orcid": "0000-0001-9765-4526" } ] }, "title": "GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2015 Published by the American Physical Society.This article is available under the terms of the Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. \n\nReceived 31 May 2016; published 15 June 2016. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max Planck Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3, Cultura i Universitats of the Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Sciences and Engineering Research Council of Canada, Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, Funda\u00e7\u00e3o de Amparo \u00e0 Pesquisa do Estado de S\u00e3o Paulo (FAPESP), Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, Ministry of Science and Technology (MOST), Taiwan, and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS and the State of Niedersachsen/Germany for provision of computational resources. \n\nThis article has been assigned the document numbers LIGO-P151226 and VIR-0285A-16.\n\nPublished - PhysRevLett.116.241103.pdf
", "abstract": "We report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) on December 26, 2015 at 03:38:53 UTC. The signal was initially identified within 70 s by an online matched-filter search targeting binary coalescences. Subsequent off-line analyses recovered GW151226 with a network signal-to-noise ratio of 13 and a significance greater than 5\u03c3. The signal persisted in the LIGO frequency band for approximately 1 s, increasing in frequency and amplitude over about 55 cycles from 35 to 450 Hz, and reached a peak gravitational strain of 3.4^(+0.7)_(-0.9) \u00d710^(-22). The inferred source-frame initial black hole masses are 14.2^(+8.3)_(-3.7) M\u2299 and 7.5^(+2.3)_(-2.3) M\u2299, and the final black hole mass is 20.8^(+6.1)_(-1.7) M\u2299. We find that at least one of the component black holes has spin greater than 0.2. This source is located at a luminosity distance of 440^(+180)_(-190)\u2009Mpc corresponding to a redshift of 0.09^(+0.03)_(-0.04). All uncertainties define a 90% credible interval. This second gravitational-wave observation provides improved constraints on stellar populations and on deviations from general relativity.", "date": "2016-06-15", "date_type": "published", "publication": "Physical Review Letters", "volume": "116", "number": "24", "publisher": "American Physical Society", "pagerange": "Art. No. 241103", "id_number": "CaltechAUTHORS:20160615-122950563", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160615-122950563", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science & Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia i Competitivitat" }, { "agency": "Conselleria d'Educaci\u00f3, Cultura i Universitats of the Govern de les Illes Balears" }, { "agency": "National Science Centre of Poland" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia e Inova\u00e7\u00e3o (MCTI)" }, { "agency": "Funda\u00e7\u00e3o de Amparo \u00e0 Pesquisa do Estado de S\u00e3o Paulo (FAPESP)" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "VIR-0285A-16", "name": "VIRGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevLett.116.241103", "primary_object": { "basename": "PhysRevLett.116.241103.pdf", "url": "https://authors.library.caltech.edu/records/qqfw7-0x416/files/PhysRevLett.116.241103.pdf" }, "resource_type": "article", "pub_year": "2016", "author_list": "Abbott, B. 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I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Engels-W", "name": { "family": "Engels", "given": "W." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Hemberger-D-A", "name": { "family": "Hemberger", "given": "D. A." } }, { "id": "Scheel-M-A", "name": { "family": "Scheel", "given": "M. A." } }, { "id": "Szilagyi-B", "name": { "family": "Szilagyi", "given": "B." } }, { "id": "Teukolsky-S-A", "name": { "family": "Teukolsky", "given": "S." }, "orcid": "0000-0001-9765-4526" } ] }, "title": "Tests of General Relativity with GW150914", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2016 American Physical Society. \n\nReceived 26 March 2016; revised manuscript received 9 May 2016; published 31 May 2016. \n\nThe authors gratefully acknowledge the support of the U.S. National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck-Society (MPS), and the State of Niedersachsen/Germany for support of the construction of Advanced LIGO and construction and operation of the GEO600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science and Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3, Cultura i Universitats of the Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Science and Engineering Research Council Canada, the Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, the Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, Ministry of Science and Technology (MOST), Taiwan, and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, and the State of Niedersachsen/Germany for the provision of computational resources. \n\nFinally, we thank the anonymous referees, whose comments helped improve the clarity of the Letter.\n\nPublished - PhysRevLett.116.221101.pdf
Submitted - 1602.03841v2.pdf
", "abstract": "The LIGO detection of GW150914 provides an unprecedented opportunity to study the two-body motion of a compact-object binary in the large-velocity, highly nonlinear regime, and to witness the final merger of the binary and the excitation of uniquely relativistic modes of the gravitational field. We carry out several investigations to determine whether GW150914 is consistent with a binary black-hole merger in general relativity. We find that the final remnant's mass and spin, as determined from the low-frequency (inspiral) and high-frequency (postinspiral) phases of the signal, are mutually consistent with the binary black-hole solution in general relativity. Furthermore, the data following the peak of GW150914 are consistent with the least-damped quasinormal mode inferred from the mass and spin of the remnant black hole. By using waveform models that allow for parametrized general-relativity violations during the inspiral and merger phases, we perform quantitative tests on the gravitational-wave phase in the dynamical regime and we determine the first empirical bounds on several high-order post-Newtonian coefficients. We constrain the graviton Compton wavelength, assuming that gravitons are dispersed in vacuum in the same way as particles with mass, obtaining a 90%-confidence lower bound of 10^(13\u2009)\u2009km. In conclusion, within our statistical uncertainties, we find no evidence for violations of general relativity in the genuinely strong-field regime of gravity.", "date": "2016-06-03", "date_type": "published", "publication": "Physical Review Letters", "volume": "116", "number": "22", "publisher": "American Physical Society", "pagerange": "Art. No. 221101", "id_number": "CaltechAUTHORS:20160607-154130083", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160607-154130083", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Engineering Research Board (SERB)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3" }, { "agency": "Cultura i Universitats of the Govern de les Illes Balears" }, { "agency": "National Science Centre of Poland" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Science and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia e Inova\u00e7\u00e3o (MCTI)" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" }, { "agency": "Ontario Ministry of Research and Innovation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevLett.116.221101", "primary_object": { "basename": "1602.03841v2.pdf", "url": "https://authors.library.caltech.edu/records/mr2zm-tzn07/files/1602.03841v2.pdf" }, "related_objects": [ { "basename": "PhysRevLett.116.221101.pdf", "url": "https://authors.library.caltech.edu/records/mr2zm-tzn07/files/PhysRevLett.116.221101.pdf" } ], "resource_type": "article", "pub_year": "2016", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/m87y8-7h044", "eprint_id": 64786, "eprint_status": "archive", "datestamp": "2023-08-22 17:32:03", "lastmod": "2023-10-17 21:52:29", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Taylor-S-R", "name": { "family": "Taylor", "given": "S. R." }, "orcid": "0000-0003-0264-1453" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Ellis-J-A", "name": { "family": "Ellis", "given": "J. A." } }, { "id": "Mingarelli-C-M-F", "name": { "family": "Mingarelli", "given": "C. M. F." }, "orcid": "0000-0002-4307-1322" }, { "id": "Lazio-T-J-W", "name": { "family": "Lazio", "given": "T. J. W." }, "orcid": "0000-0002-3873-5497" }, { "id": "van-Haasteren-R", "name": { "family": "van Haasteren", "given": "R." }, "orcid": "0000-0002-6428-2620" } ] }, "title": "Are we there yet? Time to detection of nanohertz gravitational waves based on pulsar-timing array limits", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; methods: data analysis; pulsars: general", "note": "\u00a9 2016 American Astronomical Society. \n\nReceived 2015 November 18; accepted 2016 January 21; published 2016 February 23. \n\nIt is our pleasure to thank Pablo Rosado, Alberto Sesana, Jonathan Gair, Lindley Lentati, Sarah Burke-Spolaor, Xavier Siemens, Maura McLaughlin, Joseph Romano, and Michael Kramer for very useful suggestions. We also thank the full NANOGrav collaboration for their comments and remarks. S.R.T. was supported by an appointment to the NASA Postdoctoral Program at the Jet Propulsion Laboratory, administered by Oak Ridge Associated Universities through a contract with NASA. M.V. acknowledges support from the JPL RTD program. J.A.E. and R.v.H. acknowledge support by NASA through Einstein Fellowship grants PF4-150120 and PF3-140116, respectively. C.M.F.M. was supported by a Marie Curie International Outgoing Fellowship within the European Union Seventh Framework Programme. This work was supported in part by National Science Foundation Physics Frontier Center award No. 1430284 and by grant PHYS-1066293 and the hospitality of the Aspen Center for Physics. This research was performed at the Jet Propulsion Laboratory, under contract with the National Aeronautics and Space Administration.\n\nPublished - Taylor_2016pL6.pdf
Submitted - 1511.05564v1.pdf
", "abstract": "Decade-long timing observations of arrays of millisecond pulsars have placed highly constraining upper limits on the amplitude of the nanohertz gravitational-wave stochastic signal from the mergers of supermassive black hole binaries (~10^(\u221215) strain at f = 1 yr^(\u22121)). These limits suggest that binary merger rates have been overestimated, or that environmental influences from nuclear gas or stars accelerate orbital decay, reducing the gravitational-wave signal at the lowest, most sensitive frequencies. This prompts the question whether nanohertz gravitational waves (GWs) are likely to be detected in the near future. In this Letter, we answer this question quantitatively using simple statistical estimates, deriving the range of true signal amplitudes that are compatible with current upper limits, and computing expected detection probabilities as a function of observation time. We conclude that small arrays consisting of the pulsars with the least timing noise, which yield the tightest upper limits, have discouraging prospects of making a detection in the next two decades. By contrast, we find large arrays are crucial to detection because the quadrupolar spatial correlations induced by GWs can be well sampled by many pulsar pairs. Indeed, timing programs that monitor a large and expanding set of pulsars have an ~80% probability of detecting GWs within the next 10 years, under assumptions on merger rates and environmental influences ranging from optimistic to conservative. Even in the extreme case where 90% of binaries stall before merger and environmental coupling effects diminish low-frequency gravitational-wave power, detection is delayed by at most a few years.", "date": "2016-03-01", "date_type": "published", "publication": "Astrophysical Journal Letters", "volume": "819", "number": "1", "publisher": "American Astronomical Society", "pagerange": "Art. No. L6", "id_number": "CaltechAUTHORS:20160226-073845969", "issn": "2041-8205", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160226-073845969", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "JPL/NASA Postdoctoral Program" }, { "agency": "NASA Oak Ridge Associated Universities" }, { "agency": "JPL Research and Technology Development Fund" }, { "agency": "NASA Einstein Fellowship", "grant_number": "PF4-150120" }, { "agency": "NASA Einstein Fellowship", "grant_number": "PF3-140116" }, { "agency": "Marie Curie International Outgoing Fellowship" }, { "agency": "NSF", "grant_number": "PHY-1430284" }, { "agency": "NSF", "grant_number": "PHY-1066293" }, { "agency": "NASA/JPL" } ] }, "other_numbering_system": { "items": [ { "id": "2016-34", "name": "Space Radiation Laboratory" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.3847/2041-8205/819/1/L6", "primary_object": { "basename": "Taylor_2016pL6.pdf", "url": "https://authors.library.caltech.edu/records/m87y8-7h044/files/Taylor_2016pL6.pdf" }, "related_objects": [ { "basename": "1511.05564v1.pdf", "url": "https://authors.library.caltech.edu/records/m87y8-7h044/files/1511.05564v1.pdf" } ], "resource_type": "article", "pub_year": "2016", "author_list": "Taylor, S. R.; Vallisneri, M.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/s4yyf-4vd26", "eprint_id": 64892, "eprint_status": "archive", "datestamp": "2023-08-20 10:19:12", "lastmod": "2023-10-17 21:57:29", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Abbott-T-D", "name": { "family": "Abbott", "given": "T. D." } }, { "id": "Abernathy-M-R", "name": { "family": "Abernathy", "given": "M. R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Berger-B-K", "name": { "family": "Berger", "given": "B. K." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chakraborty-R", "name": { "family": "Chakraborty", "given": "R." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Driggers-J-C", "name": { "family": "Driggers", "given": "J. C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Gushwa-K-E", "name": { "family": "Gushwa", "given": "K. E." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hall-E-D", "name": { "family": "Hall", "given": "E. D." }, "orcid": "0000-0001-9018-666X" }, { "id": "Heptonstall-A-W", "name": { "family": "Heptonstall", "given": "A. W." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Jacobson-M-B", "name": { "family": "Jacobson", "given": "M. B." } }, { "id": "Kanner-J-B", "name": { "family": "Kanner", "given": "J. B." }, "orcid": "0000-0001-8115-0577" }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Korth-W-Z", "name": { "family": "Korth", "given": "W. Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D. B." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lewis-J-B", "name": { "family": "Lewis", "given": "J. B." } }, { "id": "Li-T-G-F", "name": { "family": "Li", "given": "T. G. F." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Martynov-D-V", "name": { "family": "Martynov", "given": "D. V." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Price-L-R", "name": { "family": "Price", "given": "L. R." } }, { "id": "Quintero-E-A", "name": { "family": "Quintero", "given": "E. A." } }, { "id": "Reitze-D-H", "name": { "family": "Reitze", "given": "D. H." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Rollins-J-G", "name": { "family": "Rollins", "given": "J. G." } }, { "id": "Sachdev-S", "name": { "family": "Sachdev", "given": "S." }, "orcid": "0000-0002-2432-7070" }, { "id": "Sanchez-E", "name": { "family": "Sanchez", "given": "E." } }, { "id": "Schmidt-P", "name": { "family": "Schmidt", "given": "P." } }, { "id": "Shao-Z", "name": { "family": "Shao", "given": "Z." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-N-D", "name": { "family": "Smith", "given": "N. D." } }, { "id": "Smith-R-J-E", "name": { "family": "Smith", "given": "R. J. E." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S-E", "name": { "family": "Gossan", "given": "S. E." }, "orcid": "0000-0002-8138-9198" }, { "id": "Okounkova-M", "name": { "family": "Okounkova", "given": "M." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "First low frequency all-sky search for continuous gravitational wave signals", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2016 American Physical Society. \n\nReceived 22 October 2015; published 25 February 2016. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory, as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max Planck Society (MPS), and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN) and the French Centre National de la Recherche Scientifique (CNRS) for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Australian Research Council; the International Science Linkages program of the Commonwealth of Australia; the Council of Scientific and Industrial Research of India, Department of Science and Technology, India; Science and Engineering Research Board, India; Ministry of Human Resource Development, India; the Spanish Ministerio de Econom\u00eda y Competitividad; the Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3; Cultura i Universitats of the Govern de les Illes Balears; the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research; the National Science Centre of Poland; the European Union; the Royal Society; the Scottish Funding Council; the Scottish Universities Physics Alliance; the National Aeronautics and Space Administration; the Hungarian Scientific Research Fund; the Lyon Institute of Origins; the National Research Foundation of Korea; Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation; the National Science and Engineering Research Council Canada; the Brazilian Ministry of Science, Technology, and Innovation; the Carnegie Trust; the Leverhulme Trust; the David and Lucile Packard Foundation; the Research Corporation; and the Alfred P. Sloan Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS, and the State of Niedersachsen/Germany for the provision of computational resources. The authors are also grateful to the anonymous referees for their comments, which helped to improve the clarity of the paper.\n\nPublished - PhysRevD.93.042007.pdf
Submitted - 1510.03621v1.pdf
", "abstract": "In this paper we present the results of the first low frequency all-sky search of continuous gravitational wave signals conducted on Virgo VSR2 and VSR4 data. The search covered the full sky, a frequency range between 20 Hz and 128 Hz with a range of spin-down between \u22121.0\u00d710^(\u221210) Hz/s and +1.5\u00d710^(\u221211) Hz/s, and was based on a hierarchical approach. The starting point was a set of short Fast Fourier Transforms (FFT), of length 8192 seconds, built from the calibrated strain data. Aggressive data cleaning, both in the time and frequency domains, has been done in order to remove, as much as possible, the effect of disturbances of instrumental origin. On each dataset a number of candidates has been selected, using the FrequencyHough transform in an incoherent step. Only coincident candidates among VSR2 and VSR4 have been examined in order to strongly reduce the false alarm probability, and the most significant candidates have been selected. The criteria we have used for candidate selection and for the coincidence step greatly reduce the harmful effect of large instrumental artifacts. Selected candidates have been subject to a follow-up by constructing a new set of longer FFTs followed by a further incoherent analysis. No evidence for continuous gravitational wave signals was found, therefore we have set a population-based joint VSR2-VSR4 90% confidence level upper limit on the dimensionless gravitational wave strain in the frequency range between 20 Hz and 128 Hz. This is the first all-sky search for continuous gravitational waves conducted at frequencies below 50 Hz. We set upper limits in the range between about 10^(\u221224) and 2\u00d710^(\u221223) at most frequencies. Our upper limits on signal strain show an improvement of up to a factor of \u223c2 with respect to the results of previous all-sky searches at frequencies below 80 Hz.", "date": "2016-02-15", "date_type": "published", "publication": "Physical Review D", "volume": "93", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. 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I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S-E", "name": { "family": "Gossan", "given": "S. E." }, "orcid": "0000-0002-8138-9198" }, { "id": "Okounkova-M", "name": { "family": "Okounkova", "given": "M." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Search of the Orion spur for continuous gravitational waves using a loosely coherent algorithm on data from LIGO interferometers", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2016 American Physical Society. \n\nReceived 25 October 2015; published 17 February 2016. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u00f3n y Ciencia, the Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory document number LIGO-P1500034-v23.\n\nPublished - PhysRevD.93.042006.pdf
Submitted - 1510.03474v2.pdf
", "abstract": "We report results of a wideband search for periodic gravitational waves from isolated neutron stars within the Orion spur towards both the inner and outer regions of our Galaxy. As gravitational waves interact very weakly with matter, the search is unimpeded by dust and concentrations of stars. One search disk (A) is 6.87\u00b0 in diameter and centered on 20^h10^m54.71^s+33\u00b033\u203225.29\u2032\u2032, and the other (B) is 7.45\u00b0 in diameter and centered on 8^h35^m20.61^s\u221246\u00b049\u203225.151\u2032\u2032. We explored the frequency range of 50\u20131500 Hz and frequency derivative from 0 to \u22125\u00d710^(\u22129)\u2009\u2009Hz/s. A multistage, loosely coherent search program allowed probing more deeply than before in these two regions, while increasing coherence length with every stage. Rigorous follow-up parameters have winnowed the initial coincidence set to only 70 candidates, to be examined manually. None of those 70 candidates proved to be consistent with an isolated gravitational-wave emitter, and 95% confidence level upper limits were placed on continuous-wave strain amplitudes. Near 169 Hz we achieve our lowest 95% C.L. upper limit on the worst-case linearly polarized strain amplitude h_0 of 6.3\u00d710^(\u221225), while at the high end of our frequency range we achieve a worst-case upper limit of 3.4\u00d710^(\u221224) for all polarizations and sky locations.", "date": "2016-02-15", "date_type": "published", "publication": "Physical Review D", "volume": "93", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 042006", "id_number": "CaltechAUTHORS:20160316-065149466", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160316-065149466", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. 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E." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R" } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R. D." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wipf-C-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Observation of Gravitational Waves from a Binary Black Hole Merger", "ispublished": "pub", "full_text_status": "public", "note": "This article is available under the terms of the Creative Commons Attribution 3.0 License. Further distribution of this work must maintain attribution to the author(s) and the published article's title, journal citation, and DOI. \n\nReceived Jan 21 2016. Published 11 Feb 2016.\n\nThe authors gratefully acknowledge the support of the United States National Science Foundation (NSF) for the construction and operation of the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council (STFC) of the United Kingdom, the Max-Planck Society (MPS), and the State of Niedersachsen, Germany, for support of the construction of Advanced LIGO and construction and operation of the GEO 600 detector. Additional support for Advanced LIGO was provided by the Australian Research Council. The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS), and the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, for the construction and operation of the Virgo detector, and for the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Council of Scientific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry of Human Resource Development, India, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3, Cultura i Universitats of the Govern de les Illes Balears, the National Science Centre of Poland, the European Commission, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the Hungarian Scientific Research Fund (OTKA), the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Sciences and Engineering Research Council of Canada, Canadian Institute for Advanced Research, the Brazilian Ministry of Science, Technology, and Innovation, Russian Foundation for Basic Research, the Leverhulme Trust, the Research Corporation, Ministry of Science and Technology (MOST), Taiwan, and the Kavli Foundation. The authors gratefully acknowledge the support of the NSF, STFC, MPS, INFN, CNRS and the State of Niedersachsen, Germany, for provision of computational resources. This article has been assigned the document numbers LIGO-P150914 and VIR-0015A-16.\n\nPublished - PhysRevLett.116.061102.pdf
", "abstract": "On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0\u00d710^(\u221221). It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203\u2009000 years, equivalent to a significance greater than 5.1\u03c3. The source lies at a luminosity distance of 410 +160/\u2212180\u2009\u2009Mpc corresponding to a redshift z=0.09 +0.03/\u22120.04. In the source frame, the initial black hole masses are 36+5\u22124M_\u2299 and 29+4\u22124M_\u2299, and the final black hole mass is 62+4\u22124M\u2299, with 3.0+0.5\u22120.5M_\u2299c^2 radiated in gravitational waves. All uncertainties define 90% credible intervals. These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.", "date": "2016-02-12", "date_type": "published", "publication": "Physical Review Letters", "volume": "116", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 061102", "id_number": "CaltechAUTHORS:20160211-080913893", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160211-080913893", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck Society" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Council of Scientific and Industrial Research of India" }, { "agency": "Department of Science and Technology of India" }, { "agency": "Science and Engineering Research Board of India" }, { "agency": "Ministry of Human Resource Development, India" }, { "agency": "Ministerio de Economia y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia i Competitivitat" }, { "agency": "National Science Centre of Poland" }, { "agency": "European Commission" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Canadian Institute for Advanced Research (CIAR)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia e Inova\u00e7\u00e3o" }, { "agency": "Russian Foundation for Basic Research" }, { "agency": "Leverhulme Trust" }, { "agency": "Research Corporation" }, { "agency": "Ministry of Science and Technology (Taipei)" }, { "agency": "Kavli Foundation" }, { "agency": "Conselleria d'Educaci\u00f3, Cultura i Universitats of the Govern de les Illes Balears" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "State of Niedersachsen/Germany" } ] }, "other_numbering_system": { "items": [ { "id": "VIR-0015A-16", "name": "VIRGO" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevLett.116.061102", "primary_object": { "basename": "PhysRevLett.116.061102.pdf", "url": "https://authors.library.caltech.edu/records/tqmx3-ke904/files/PhysRevLett.116.061102.pdf" }, "resource_type": "article", "pub_year": "2016", "author_list": "Thorne, K. S.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/h358s-cc927", "eprint_id": 64190, "eprint_status": "archive", "datestamp": "2023-08-19 13:43:29", "lastmod": "2023-10-17 19:35:03", "type": "monograph", "metadata_visibility": "show", "creators": { "items": [ { "id": "Djorgovski-S-G", "name": { "family": "Djorgovski", "given": "S. G." }, "orcid": "0000-0002-0603-3087" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "Curt" } }, { "id": "Elmegreen-B-G", "name": { "family": "Elmegreen", "given": "Bruce G." }, "orcid": "0000-0002-1723-6330" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Mahabal-A-A", "name": { "family": "Mahabal", "given": "A." }, "orcid": "0000-0003-2242-0244" } ] }, "title": "Digging Deeper: Algorithms for Computationally-Limited Searches in Astronomy", "ispublished": "unpub", "full_text_status": "public", "note": "Accepted Version - digging_final_report.pdf
", "abstract": "Astronomy, like most other fields, is being deluged by exponentially growing streams of ever more complex data. While these massive data streams bring a great discovery potential, their full scientific exploitation poses many challenges, due to both data volumes and data complexity.\nMoreover, the need to discover and characterize interesting, faint signals in such data streams quickly and robustly, in order to deploy costly follow-up resources that are often necessary for\nthe full scientific returns, makes the challenges even sharper. Examples in astronomy include transient events and variable sources found in digital synoptic sky surveys, gravitational wave signals, faint radio transients, pulsars, and other types of variable sources in the next generation of panoramic radio surveys, etc. Similar situations arise in the context of space science and planetary exploration, environmental monitoring, security, etc. In most cases, rapid discovery\nand characterization of interesting signals is highly computationally limited. The goal of this study was to define a number of interesting, often mission-critical challenges of this nature in the\nbroader context of time-domain astronomy, but with an eye on their applicability elsewhere.", "date": "2016-02-04", "date_type": "published", "publisher": "Keck Institute for Space Studies", "id_number": "CaltechAUTHORS:20160203-094000654", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160203-094000654", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "Keck Institute for Space Studies (KISS)" } ] }, "local_group": { "items": [ { "id": "Keck-Institute-for-Space-Studies" } ] }, "doi": "10.26206/S5YB-TR47", "primary_object": { "basename": "digging_final_report.pdf", "url": "https://authors.library.caltech.edu/records/h358s-cc927/files/digging_final_report.pdf" }, "resource_type": "monograph", "pub_year": "2016", "author_list": "Djorgovski, S. G.; Cutler, Curt; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/nr7yw-q9p11", "eprint_id": 58405, "eprint_status": "archive", "datestamp": "2023-08-20 06:52:35", "lastmod": "2023-10-23 19:19:07", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Abernathy-M-R", "name": { "family": "Abernathy", "given": "M. R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-R-A", "name": { "family": "Anderson", "given": "R. A." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Austin-L", "name": { "family": "Austin", "given": "L." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. 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I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. 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D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } } ] }, "title": "Characterization of the LIGO detectors during their sixth science run", "ispublished": "pub", "full_text_status": "public", "keywords": "LIGO, gravitational waves, detector characterization", "note": "\u00a9 2015 IOP Publishing Ltd. Received 18 November 2014, revised 12 March 2015. Accepted for publication 31 March 2015. Published 13 May 2015.\n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the\nFoundation for Fundamental Research on Matter supported by the Netherlands Organization for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P Sloan Foundation.\n\nSubmitted - 1410.7764v2.pdf
", "abstract": "In 2009\u20132010, the Laser Interferometer Gravitational-Wave Observatory (LIGO) operated together with international partners Virgo and GEO600 as a network to search for gravitational waves (GWs) of astrophysical origin. The sensitivity of these detectors was limited by a combination of noise sources inherent to the instrumental design and its environment, often localized in time or frequency, that couple into the GW readout. Here we review the performance of the LIGO instruments during this epoch, the work done to characterize the detectors and their data, and the effect that transient and continuous noise artefacts have on the sensitivity of LIGO to a variety of astrophysical sources.", "date": "2015-06-11", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "32", "number": "11", "publisher": "IOP", "pagerange": "Art. No. 115012", "id_number": "CaltechAUTHORS:20150622-120844267", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150622-120844267", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" } ] }, "other_numbering_system": { "items": [ { "id": "2015-39", "name": "Space Radiation Laboratory" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "TAPIR" }, { "id": "Space-Radiation-Laboratory" } ] }, "doi": "10.1088/0264-9381/32/11/115012", "primary_object": { "basename": "1410.7764v2.pdf", "url": "https://authors.library.caltech.edu/records/nr7yw-q9p11/files/1410.7764v2.pdf" }, "resource_type": "article", "pub_year": "2015", "author_list": "Aasi, J.; Abadie, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/xsg32-t7248", "eprint_id": 59539, "eprint_status": "archive", "datestamp": "2023-08-20 06:15:36", "lastmod": "2023-10-23 20:42:25", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" }, { "id": "Kanner-J-B", "name": { "family": "Kanner", "given": "Jonah" }, "orcid": "0000-0001-8115-0577" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "Roy" }, "orcid": "0000-0002-9145-8580" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan" }, "orcid": "0000-0002-0928-6784" }, { "id": "Stephens-B", "name": { "family": "Stephens", "given": "Branson" } } ] }, "title": "The LIGO Open Science Center", "ispublished": "pub", "full_text_status": "public", "note": "Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. \n\nWe thank Stuart Anderson, Juan Barayoga, Patrick Brady, Duncan Brown, Laura Cadonati, Vuk Mandic, Szabi Marka, Greg Mendell, Keith Riles, Peter Shawhan, David Shoemaker, and Eric Thrane for helpful discussions and interactions. Beverly Berger, Marie-Anne Bizouard, Vicki Kalogera, Andrew Lundgren, Vivien Raymond, and John Whelan participated in the LSC review of the S5 dataset. We are grateful to the Virgo and GEO collaborations for allowing the LOSC Timeline tool to report observation-segment metadata for their detectors. Alexander Cole, Ashley Disbrow, Gary LaMotte, and Shannon Wang performed early tests of the data. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation, and operates under cooperative agreement NSF-0757058. The LIGO Open Science Center (LOSC) was partially funded by grant NSF-1210172. Part of this work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract to the National Aeronautics and Space Administration. This is LIGO document LIGO-P1400186. Copyright 2014.\n\nPublished - 1742-6596_610_1_012021.pdf
", "abstract": "The LIGO Open Science Center (LOSC) fulfills LIGO's commitment to release, archive, and serve LIGO data in a broadly accessible way to the scientific community and to the public, and to provide the information and tools necessary to understand and use the data. In August 2014, the LOSC published the full dataset from Initial LIGO's \"S5\" run at design sensitivity, the first such large-scale release and a valuable testbed to explore the use of LIGO data by non-LIGO researchers and by the public, and to help teach gravitational-wave data analysis to students across the world. In addition to serving the S5 data, the LOSC web portal (losc.ligo.org) now offers documentation, data-location and data-quality queries, tutorials and example code, and more. We review the mission and plans of the LOSC, focusing on the S5 data release.", "date": "2015-05-11", "date_type": "published", "publication": "Journal of Physics: Conference Series", "volume": "610", "publisher": "IOP", "pagerange": "Art. No. 012021", "id_number": "CaltechAUTHORS:20150814-114443011", "issn": "1742-6596", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150814-114443011", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "NSF-0757058" }, { "agency": "NSF", "grant_number": "NSF-1210172" }, { "agency": "NASA/JPL/Caltech" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1400186", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "doi": "10.1088/1742-6596/610/1/012021", "primary_object": { "basename": "1742-6596_610_1_012021.pdf", "url": "https://authors.library.caltech.edu/records/xsg32-t7248/files/1742-6596_610_1_012021.pdf" }, "resource_type": "article", "pub_year": "2015", "author_list": "Vallisneri, Michele; Kanner, Jonah; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/1h5jb-9zv53", "eprint_id": 56746, "eprint_status": "archive", "datestamp": "2023-08-20 05:47:16", "lastmod": "2023-10-23 15:47:12", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chakraborty-R", "name": { "family": "Chakraborty", "given": "R." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "Driggers-J-C", "name": { "family": "Driggers", "given": "J. C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Gushwa-K-E", "name": { "family": "Gushwa", "given": "K." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. 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R." } }, { "id": "Smith-R-J-E", "name": { "family": "Smith", "given": "R. J. E." } }, { "id": "Smith-Lefebvre-N-D", "name": { "family": "Smith-Lefebvre", "given": "N. D." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Thrane-E", "name": { "family": "Thrane", "given": "E." }, "orcid": "0000-0002-4418-3895" }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Nissanke-S", "name": { "family": "Nissanke", "given": "S." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Advanced LIGO", "ispublished": "pub", "full_text_status": "restricted", "keywords": "gravitational waves, interferometers, seismic isolation, optics", "note": "\u00a9 2015 IOP Publishing Ltd. Received 11 November 2014, revised 12 December 2014. Accepted for publication 30 December 2014. Published 3 March 2015. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages programme of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia, Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, OTKA of Hungary, the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This article has LIGO document number LIGO-P1400177.", "abstract": "The Advanced LIGO gravitational wave detectors are second-generation instruments designed and built for the two LIGO observatories in Hanford, WA and Livingston, LA, USA. The two instruments are identical in design, and are specialized versions of a Michelson interferometer with 4 km long arms. As in Initial LIGO, Fabry\u2013Perot cavities are used in the arms to increase the interaction time with a gravitational wave, and power recycling is used to increase the effective laser power. Signal recycling has been added in Advanced LIGO to improve the frequency response. In the most sensitive frequency region around 100 Hz, the design strain sensitivity is a factor of 10 better than Initial LIGO. In addition, the low frequency end of the sensitivity band is moved from 40 Hz down to 10 Hz. All interferometer components have been replaced with improved technologies to achieve this sensitivity gain. Much better seismic isolation and test mass suspensions are responsible for the gains at lower frequencies. Higher laser power, larger test masses and improved mirror coatings lead to the improved sensitivity at mid and high frequencies. Data collecting runs with these new instruments are planned to begin in mid-2015.", "date": "2015-04-09", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "32", "number": "7", "publisher": "IOP", "pagerange": "Art. No. 074001", "id_number": "CaltechAUTHORS:20150417-133457450", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150417-133457450", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages programme of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Ontario Ministry of Research and Innovation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1400177", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1088/0264-9381/32/7/074001", "resource_type": "article", "pub_year": "2015", "author_list": "Aasi, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/vrpe1-f7489", "eprint_id": 57179, "eprint_status": "archive", "datestamp": "2023-08-20 05:26:23", "lastmod": "2023-10-23 17:07:58", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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D." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Thrane-E", "name": { "family": "Thrane", "given": "E." }, "orcid": "0000-0002-4418-3895" }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Nissanke-S", "name": { "family": "Nissanke", "given": "S." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Directed search for gravitational waves from Scorpius X-1 with initial LIGO data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2015 American Physical Society. Received 3 December 2014; published 26 March 2015.\n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation (NSF) for the\nconstruction and operation of the LIGO Laboratory,\nthe Science and Technology Facilities Council (STFC)\nof the United Kingdom, the Max-Planck-Society (MPS),\nand the State of Niedersachsen/Germany for support of\nthe construction and operation of the GEO600 detector, the\nItalian Istituto Nazionale di Fisica Nucleare (INFN) and the\nFrench Centre National de la Recherche Scientifique\n(CNRS) for the construction and operation of the Virgo\ndetector and the creation and support of the EGO consortium.\nThe authors also gratefully acknowledge research\nsupport from these agencies as well as by the Australian\nResearch Council, the International Science Linkages\nprogram of the Commonwealth of Australia, the Council\nof Scientific and Industrial Research of India, Department\nof Science and Technology, India, Science & Engineering\nResearch Board (SERB), India, Ministry of Human\nResource Development, India, the Spanish Ministerio de\nEconom\u00eda y Competitividad, the Conselleria d'Economia i\nCompetitivitat and Conselleria d'Educaci\u00f3, Cultura i\nUniversitats of the Govern de les Illes Balears, the\nFoundation for Fundamental Research on Matter supported\nby the Netherlands Organisation for Scientific Research,\nthe Polish Ministry of Science and Higher Education, the\nFOCUS Programme of Foundation for Polish Science, the\nEuropean Union, the Royal Society, the Scottish Funding\nCouncil, the Scottish Universities Physics Alliance, the\nNational Aeronautics and Space Administration, the\nHungarian Scientific Research Fund (OTKA), the Lyon\nInstitute of Origins (LIO), the National Research\nFoundation of Korea, Industry Canada and the Province\nof Ontario through the Ministry of Economic Development\nand Innovation, the National Science and Engineering\nResearch Council Canada, the Brazilian Ministry of\nScience, Technology, and Innovation, the Carnegie Trust,\nthe Leverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation, and the Alfred P.\nSloan Foundation. The authors gratefully acknowledge the\nsupport of the NSF, STFC, MPS, INFN, CNRS and the\nState of Niedersachsen/Germany for provision of computational\nresources.\n\nPublished - PhysRevD.91.062008.pdf
Submitted - 1412.0605v1.pdf
", "abstract": "We present results of a search for continuously emitted gravitational radiation, directed at the brightest low-mass x-ray binary, Scorpius X-1. Our semicoherent analysis covers 10 days of LIGO S5 data ranging from 50\u2013550 Hz, and performs an incoherent sum of coherent F-statistic power distributed amongst frequency-modulated orbital sidebands. All candidates not removed at the veto stage were found to be consistent with noise at a 1% false alarm rate. We present Bayesian 95% confidence upper limits on gravitational-wave strain amplitude using two different prior distributions: a standard one, with no a priori assumptions about the orientation of Scorpius X-1; and an angle-restricted one, using a prior derived from electromagnetic observations. Median strain upper limits of 1.3\u00d710^(\u221224) and 8\u00d710^(\u221225) are reported at 150 Hz for the standard and angle-restricted searches respectively. This proof-of-principle analysis was limited to a short observation time by unknown effects of accretion on the intrinsic spin frequency of the neutron star, but improves upon previous upper limits by factors of \u223c1.4 for the standard, and 2.3 for the angle-restricted search at the sensitive region of the detector.", "date": "2015-03-15", "date_type": "published", "publication": "Physical Review D", "volume": "91", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 062008", "id_number": "CaltechAUTHORS:20150504-084613268", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150504-084613268", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society and the State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Ministry of Human Resource Development (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia i Competitivitat and Conselleria d'Educaci\u00f3" }, { "agency": "Cultura i Universitats of the Govern de les Illes Balears" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "European Union" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Hungarian Scientific Research Foundation (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Minist\u00e9rio da Ci\u00eancia, Tecnologia, Inova\u00e7\u00e3o e Comunica\u00e7\u00e3o" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Ontario Ministry of Research and Innovation" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.91.062008", "primary_object": { "basename": "1412.0605v1.pdf", "url": "https://authors.library.caltech.edu/records/vrpe1-f7489/files/1412.0605v1.pdf" }, "related_objects": [ { "basename": "PhysRevD.91.062008.pdf", "url": "https://authors.library.caltech.edu/records/vrpe1-f7489/files/PhysRevD.91.062008.pdf" } ], "resource_type": "article", "pub_year": "2015", "author_list": "Aasi, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/e6sm4-n7r94", "eprint_id": 55686, "eprint_status": "archive", "datestamp": "2023-08-20 04:36:30", "lastmod": "2023-10-20 22:58:16", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Abernathy-M-R", "name": { "family": "Abernathy", "given": "M. R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. 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E." } }, { "id": "Smith-Lefebvre-N-D", "name": { "family": "Smith-Lefebvre", "given": "N. D." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Thrane-E", "name": { "family": "Thrane", "given": "E." }, "orcid": "0000-0002-4418-3895" }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vajente-G", "name": { "family": "Vajente", "given": "G." }, "orcid": "0000-0002-7656-6882" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Nissanke-S", "name": { "family": "Nissanke", "given": "S." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2015 American Physical Society. Received 7 November 2014; published 21 January 2015.\n\nThe authors thank the anonymous referee for the careful reading of the manuscript. They also gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, OTKA of Hungary, the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the Natural Sciences and Engineering Research Council of Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - PhysRevD.91.022004.pdf
Submitted - 1410.8310v1.pdf
", "abstract": "In this paper we present the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data. In order to take into account a possible small mismatch between the gravitational-wave frequency and two times the star rotation frequency, inferred from measurement of the electromagnetic pulse rate, a range of 0.02 Hz around two times the star rotational frequency has been searched for both the pulsars. No evidence for a signal has been found and 95% confidence level upper limits have been computed assuming both that polarization parameters are completely unknown and that they are known with some uncertainty, as derived from x-ray observations of the pulsar wind torii. For Vela the upper limits are comparable to the spin-down limit, computed assuming that all the observed spin-down is due to the emission of gravitational waves. For Crab the upper limits are about a factor of 2 below the spin-down limit, and represent a significant improvement with respect to past analysis. This is the first time the spin-down limit is significantly overcome in a narrow-band search.", "date": "2015-01-15", "date_type": "published", "publication": "Physical Review D", "volume": "91", "number": "2", "publisher": "American Physical Society", "pagerange": "Art. No. 022004", "id_number": "CaltechAUTHORS:20150310-151957061", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150310-151957061", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Spanish Ministerio de Econom\u00eda y Competitividad" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "NASA" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Ontario Ministry of Research and Innovation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.91.022004", "primary_object": { "basename": "1410.8310v1.pdf", "url": "https://authors.library.caltech.edu/records/e6sm4-n7r94/files/1410.8310v1.pdf" }, "related_objects": [ { "basename": "PhysRevD.91.022004.pdf", "url": "https://authors.library.caltech.edu/records/e6sm4-n7r94/files/PhysRevD.91.022004.pdf" } ], "resource_type": "article", "pub_year": "2015", "author_list": "Aasi, J.; Abbott, B. 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G." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Singer-L", "name": { "family": "Singer", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Smith-Lefebvre-N-D", "name": { "family": "Smith-Lefebvre", "given": "N. D." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Thrane-E", "name": { "family": "Thrane", "given": "E." }, "orcid": "0000-0002-4418-3895" }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Hong-T", "name": { "family": "Hong", "given": "T." } }, { "id": "Kaufman-K", "name": { "family": "Kaufman", "given": "K." } }, { "id": "Luan-Jing", "name": { "family": "Luan", "given": "J." }, "orcid": "0000-0001-6048-1959" }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } } ] }, "title": "Searching for stochastic gravitational waves using data from the two colocated LIGO Hanford detectors", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2015 American Physical Society. Received 4 November 2014; published 8 January 2015.\n\nThe authors gratefully acknowledge the support of the U.S. National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science\nLinkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria\nd'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, OTKA of Hungary, the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - PhysRevD.91.022003.pdf
Submitted - 1410.6211v3.pdf
", "abstract": "Searches for a stochastic gravitational-wave background (SGWB) using terrestrial detectors typically involve cross-correlating data from pairs of detectors. The sensitivity of such cross-correlation analyses depends, among other things, on the separation between the two detectors: the smaller the separation, the better the sensitivity. Hence, a colocated detector pair is more sensitive to a gravitational-wave background than a noncolocated detector pair. However, colocated detectors are also expected to suffer from correlated noise from instrumental and environmental effects that could contaminate the measurement of the background. Hence, methods to identify and mitigate the effects of correlated noise are necessary to achieve the potential increase in sensitivity of colocated detectors. Here we report on the first SGWB analysis using the two LIGO Hanford detectors and address the complications arising from correlated environmental noise. We apply correlated noise identification and mitigation techniques to data taken by the two LIGO Hanford detectors, H1 and H2, during LIGO's fifth science run. At low frequencies, 40\u2013460 Hz, we are unable to sufficiently mitigate the correlated noise to a level where we may confidently measure or bound the stochastic gravitational-wave signal. However, at high frequencies, 460\u20131000 Hz, these techniques are sufficient to set a 95% confidence level upper limit on the gravitational-wave energy density of \u03a9(f)<7.7\u00d710^(\u22124)(f/900\u2009\u2009Hz)^3, which improves on the previous upper limit by a factor of \u223c180. In doing so, we demonstrate techniques that will be useful for future searches using advanced detectors, where correlated noise (e.g., from global magnetic fields) may affect even widely separated detectors.", "date": "2015-01-15", "date_type": "published", "publication": "Physical Review D", "volume": "91", "number": "2", "publisher": "American Physical Society", "pagerange": "Art. No. 022003", "id_number": "CaltechAUTHORS:20150317-110958591", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150317-110958591", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Max-Planck-Society" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ontario Ministry of Research and Innovation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.91.022003", "primary_object": { "basename": "1410.6211v3.pdf", "url": "https://authors.library.caltech.edu/records/878mm-zs775/files/1410.6211v3.pdf" }, "related_objects": [ { "basename": "PhysRevD.91.022003.pdf", "url": "https://authors.library.caltech.edu/records/878mm-zs775/files/PhysRevD.91.022003.pdf" } ], "resource_type": "article", "pub_year": "2015", "author_list": "Aasi, J.; Abadie, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/ndfkh-7vt52", "eprint_id": 53285, "eprint_status": "archive", "datestamp": "2023-08-20 03:58:41", "lastmod": "2023-10-19 14:43:51", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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D." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Thrane-E", "name": { "family": "Thrane", "given": "E." }, "orcid": "0000-0002-4418-3895" }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "M\u00f6sta-P", "name": { "family": "Moesta", "given": "P." }, "orcid": "0000-0002-9371-1447" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Reitze-D-H", "name": { "family": "Reitze", "given": "D. H." } } ] }, "title": "Improved Upper Limits on the Stochastic Gravitational-Wave Background from 2009\u20132010 LIGO and Virgo Data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2014 American Physical Society. \n\nReceived 7 July 2014; published 2 December 2014. \n\nThe authors gratefully acknowledge the support of the U. S. National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and\nTechnology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen, Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge\nthe support of the research by these agencies and by \nthe Australian Research Council, the International Science\nLinkages program of the Commonwealth of Australia, the\nCouncil of Scientific and Industrial Research of India, the\nIstituto Nazionale di Fisica Nucleare of Italy, the Spanish\nMinisterio de Econom\u00eda y Competitividad, the Conselleria\nd'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes\nBalears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the National Aeronautics and Space Administration, the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and\nInnovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, the OTKA of Hungary, the Science and Technologies Funding Council of the UK, the Lyon Institute of Origins (LIO), and the Alfred P. Sloan Foundation.\n\nPublished - PhysRevLett.113.231101.pdf
Submitted - 1406.4556v2.pdf
", "abstract": "Gravitational waves from a variety of sources are predicted to superpose to create a stochastic background. This background is expected to contain unique information from throughout the history of the Universe that is unavailable through standard electromagnetic observations, making its study of fundamental importance to understanding the evolution of the Universe. We carry out a search for the stochastic background with the latest data from the LIGO and Virgo detectors. Consistent with predictions from most stochastic gravitational-wave background models, the data display no evidence of a stochastic gravitational-wave signal. Assuming a gravitational-wave spectrum of \u03a9_(GW)(f)=\u03a9_\u03b1(f/f_(ref))_\u03b1, we place 95% confidence level upper limits on the energy density of the background in each of four frequency bands spanning 41.5\u20131726 Hz. In the frequency band of 41.5\u2013169.25 Hz for a spectral index of \u03b1=0, we constrain the energy density of the stochastic background to be \u03a9_(GW)(f)<5.6\u00d710^(\u22126). For the 600\u20131000 Hz band, \u03a9_(GW)(f)<0.14(f/900\u2009\u2009Hz)^3, a factor of 2.5 lower than the best previously reported upper limits. We find \u03a9_(GW)(f)<1.8\u00d710^(\u22124) using a spectral index of zero for 170\u2013600 Hz and \u03a9_(GW)(f)<1.0(f/1300\u2009\u2009Hz)^3 for 1000\u20131726 Hz, bands in which no previous direct limits have been placed. The limits in these four bands are the lowest direct measurements to date on the stochastic background. We discuss the implications of these results in light of the recent claim by the BICEP2 experiment of the possible evidence for inflationary gravitational waves.", "date": "2014-12-05", "date_type": "published", "publication": "Physical Review Letters", "volume": "113", "number": "23", "publisher": "American Physical Society", "pagerange": "Art. No. 231101", "id_number": "CaltechAUTHORS:20150107-131249161", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150107-131249161", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Australian Research Council" }, { "agency": "Commonwealth of Australia International Science Linkages Program" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Ontario Ministry of Research and Innovation" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevLett.113.231101", "primary_object": { "basename": "1406.4556v2.pdf", "url": "https://authors.library.caltech.edu/records/ndfkh-7vt52/files/1406.4556v2.pdf" }, "related_objects": [ { "basename": "PhysRevLett.113.231101.pdf", "url": "https://authors.library.caltech.edu/records/ndfkh-7vt52/files/PhysRevLett.113.231101.pdf" } ], "resource_type": "article", "pub_year": "2014", "author_list": "Aasi, J.; Abbott, B. 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J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "Nissanke-S", "name": { "family": "Nissanke", "given": "S." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } } ] }, "title": "Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2014 American Physical Society. Received 14 July 2014; published 17 November 2014.\n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector, and the Italian\nIstituto Nazionale di Fisica Nucleare and the French Centre\nNational de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors also\ngratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported\nby the Netherlands Organisation for Scientific Research,\nthe Polish Ministry of Science and Higher Education, the\nFOCUS Programme of Foundation for Polish Science, the\nRoyal Society, the Scottish Funding Council, the Scottish\nUniversities Physics Alliance, The National Aeronautics\nand Space Administration, Hungarian Scientific Research\nFund, the Lyon Institute of Origins (LIO), the National\nResearch Foundation of Korea, Industry Canada and the\nProvince of Ontario through the Ministry of Economic\nDevelopment and Innovation, the National Science and\nEngineering Research Council Canada, the Carnegie Trust,\nthe Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P.\nSloan Foundation. This article has LIGO document number\nLIGO-P1400046. We acknowledge the support from the following agencies: U.S. National Science Foundation-\nOffice of Polar Programs, U.S. National Science\nFoundation-Physics Division, University of Wisconsin\nAlumni Research Foundation, the Grid Laboratory Of\nWisconsin (GLOW) grid infrastructure at the University\nof Wisconsin, Madison; the Open Science Grid (OSG) grid\ninfrastructure; U.S. Department of Energy, and National\nEnergy Research Scientific Computing Center, the\nLouisiana Optical Network Initiative (LONI) grid computing\nresources; Natural Sciences and Engineering\nResearch Council of Canada, WestGrid and Compute/\nCalcul Canada; Swedish Research Council, Swedish\nPolar Research Secretariat, Swedish National\nInfrastructure for Computing (SNIC), and Knut and\nAlice Wallenberg Foundation, Sweden; German Ministry\nfor Education and Research (BMBF), Deutsche\nForschungsgemeinschaft (DFG), Helmholtz Alliance for\nAstroparticle Physics (HAP), Research Department of\nPlasmas with Complex Interactions (Bochum), Germany;\nFund for Scientific Research (FNRS-FWO), FWO\nOdysseus programme, Flanders Institute to encourage\nscientific and technological research in industry (IWT),\nBelgian Federal Science Policy Office (Belspo); University\nof Oxford, U.K.; Marsden Fund, New Zealand; Australian\nResearch Council; Japan Society for Promotion of Science\n(JSPS); the Swiss National Science Foundation (SNSF),\nSwitzerland; National Research Foundation of Korea (NRF);\nDanish National Research Foundation, Denmark (DNRF).\n\nPublished - PhysRevD.90.102002.pdf
Submitted - 1407.1042v2.pdf
", "abstract": "We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007\u20132010. These include parts of the 2005\u20132007 run and the 2009\u20132010 run for LIGO-Virgo, and IceCube's observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of gravitational-wave emission energy of 10^(\u22122)\u2009\u2009M_\u2299c^2 at \u223c150\u2009\u2009Hz with \u223c60\u2009\u2009ms duration, and high-energy neutrino emission of 10^(51)\u2009\u2009erg comparable to the isotropic gamma-ray energy of gamma-ray bursts, we limit the source rate below 1.6\u00d710^(\u22122)\u2009\u2009Mpc^(\u22123)\u2009yr^(\u22121). We also examine how combining information from gravitational waves and neutrinos will aid discovery in the advanced gravitational-wave detector era.", "date": "2014-11-15", "date_type": "published", "publication": "Physical Review D", "volume": "90", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102002", "id_number": "CaltechAUTHORS:20150108-091905659", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150108-091905659", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Australian Research Council" }, { "agency": "Commonwealth of Australia International Science Linkages Program" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "NSF" }, { "agency": "University of Wisconsin Alumni Research Foundation" }, { "agency": "University of Wisconsin, Madison Grid Laboratory Of Wisconsin (GLOW)" }, { "agency": "Open Science Grid (OSG)" }, { "agency": "Department of Energy (DOE)" }, { "agency": "National Energy Research Scientific Computing Center" }, { "agency": "Louisiana Optical Network Initiative (LONI)" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "WestGrid and Compute/Calcul Canada" }, { "agency": "Swedish Research Council" }, { "agency": "Swedish Polar Research Secretariat" }, { "agency": "Swedish National Infrastructure for Computing (SNIC)" }, { "agency": "Knut and Alice Wallenberg Foundation" }, { "agency": "Bundesministerium f\u00fcr Bildung und Forschung (BMBF)" }, { "agency": "Deutsche Forschungsgemeinschaft (DFG)" }, { "agency": "Helmholtz Alliance for Astroparticle Physics" }, { "agency": "Research Department of Plasmas with Complex Interactions (Bochum), Germany" }, { "agency": "Fonds de la Recherche Scientifique (FNRS)" }, { "agency": "Fonds Wetenschappelijk Onderzoek - Vlaanderen (FWO)" }, { "agency": "Fonds pour la Formation \u00e0 la Recherche dans l'\u00edndustrie et dans l'\u00c1griculture (FRIA-Belgium)" }, { "agency": "University of Oxford, U.K." }, { "agency": "Marsden Fund, New Zealand" }, { "agency": "Australian Research Council" }, { "agency": "Japan Society for Promotion of Science (JSPS)" }, { "agency": "Swiss National Science Foundation (SNSF)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Danish National Research Foundation" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Ontario Ministry of Research and Innovation" } ] }, "other_numbering_system": { "items": [ { "id": "P1400046", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "IceCube Collaboration", "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.90.102002", "primary_object": { "basename": "1407.1042v2.pdf", "url": "https://authors.library.caltech.edu/records/dzmkk-4z846/files/1407.1042v2.pdf" }, "related_objects": [ { "basename": "PhysRevD.90.102002.pdf", "url": "https://authors.library.caltech.edu/records/dzmkk-4z846/files/PhysRevD.90.102002.pdf" } ], "resource_type": "article", "pub_year": "2014", "author_list": "Aartsen, M. G.; Aasi, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/84qzv-zk851", "eprint_id": 50760, "eprint_status": "archive", "datestamp": "2023-08-20 02:57:31", "lastmod": "2023-10-18 14:28:29", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Abernathy-M-R", "name": { "family": "Abernathy", "given": "M. R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-R", "name": { "family": "Anderson", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Austin-L", "name": { "family": "Austin", "given": "L." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. 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I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "M\u00f6sta-P", "name": { "family": "Moesta", "given": "P." }, "orcid": "0000-0002-9371-1447" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } } ] }, "title": "First all-sky search for continuous gravitational waves from unknown sources in binary systems", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2014 American Physical Society.\n\nReceived 9 June 2014; Published 15 September 2014.\n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory; the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector; and the Italian\nIstituto Nazionale di Fisica Nucleare and the French Centre\nNational de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors also\ngratefully acknowledge the support of the research by\nthese agencies and by the Australian Research Council, the\nInternational Science Linkages program of the\nCommonwealth of Australia, the Council of Scientific\nand Industrial Research of India, the Istituto Nazionale\ndi Fisica Nucleare of Italy, the Spanish Ministerio de\nEconom\u00eda y Competitividad, the Conselleria d'Economia\nHisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the\nFoundation for Fundamental Research on Matter supported\nby the Netherlands Organisation for Scientific Research,\nthe Polish Ministry of Science and Higher Education, the\nFOCUS Programme of Foundation for Polish Science, the\nRoyal Society, the Scottish Funding Council, the Scottish\nUniversities Physics Alliance, the National Aeronautics\nand Space Administration, OTKA of Hungary, the Lyon\nInstitute of Origins (LIO), the National Research\nFoundation of Korea, Industry Canada and the Province\nof Ontario through the Ministry of Economic Development\nand Innovation, the National Science and Engineering\nResearch Council Canada, the Carnegie Trust, the\nLeverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation, and the Alfred P.\nSloan Foundation. This article has LIGO Document\nNo. LIGO-P1300048.\n\nPublished - PhysRevD.90.062010.pdf
Submitted - 1405.7904v2.pdf
", "abstract": "We present the first results of an all-sky search for continuous gravitational waves from unknown spinning neutron stars in binary systems using LIGO and Virgo data. Using a specially developed analysis program, the TwoSpect algorithm, the search was carried out on data from the sixth LIGO science run and the second and third Virgo science runs. The search covers a range of frequencies from 20 Hz to 520 Hz, a range of orbital periods from 2 to \u223c2,254\u2009\u2009h and a frequency- and period-dependent range of frequency modulation depths from 0.277 to 100 mHz. This corresponds to a range of projected semimajor axes of the orbit from \u223c0.6\u00d710^(\u22123) \u2009ls to \u223c6,500\u2009\u2009ls assuming the orbit of the binary is circular. While no plausible candidate gravitational wave events survive the pipeline, upper limits are set on the analyzed data. The most sensitive 95% confidence upper limit obtained on gravitational wave strain is 2.3\u00d710^(\u221224) at 217 Hz, assuming the source waves are circularly polarized. Although this search has been optimized for circular binary orbits, the upper limits obtained remain valid for orbital eccentricities as large as 0.9. In addition, upper limits are placed on continuous gravitational wave emission from the low-mass x-ray binary Scorpius X-1 between 20 Hz and 57.25 Hz.", "date": "2014-09-15", "date_type": "published", "publication": "Physical Review D", "volume": "90", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. 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S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } } ] }, "title": "Implementation of an F-statistic all-sky search for continuous gravitational waves in Virgo VSR1 data", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; gravitational radiation detectors; pulsars; data analysis: algorithms and implementation", "note": "\u00a9 2014 IOP Publishing Ltd. \n\nReceived 7 March 2014; Revised 16 June 2014; Accepted for publication 2 July 2014; Published 5 August 2014. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth\nof Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d\u02bcEconomia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the PL-Grid Infrastructure, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P Sloan Foundation. This document has been assigned LIGO Laboratory document number LIGO-P1300133.\n\nSubmitted - 1402.4974v3.pdf
", "abstract": "We present an implementation of the F-statistic to carry out the first search in data from the Virgo laser interferometric gravitational wave detector for periodic gravitational waves from a priori unknown, isolated rotating neutron stars. We searched a frequency f_0 range from 100 Hz to 1 kHz and the frequency dependent spindown f_1 range from -1.6(f_0/100 Hz) x 10^(-9) Hz s^(\u22121) to zero. A large part of this frequency\u2013spindown space was unexplored by any of the all-sky searches published so far. Our method consisted of a coherent search over two-day periods using the F-statistic, followed by a search for coincidences among the candidates from the two-day segments. We have introduced a number of novel techniques and algorithms that allow the use of the fast Fourier transform (FFT) algorithm in the coherent part of the search resulting in a fifty-fold speed-up in computation of the F-statistic with respect to the algorithm used in the other pipelines. No significant gravitational wave signal was found. The sensitivity of the search was estimated by injecting signals into the data. In the most sensitive parts of the detector band more than 90% of signals would have been detected with dimensionless gravitational-wave amplitude greater than 5 x 10^(-24).", "date": "2014-08-21", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "31", "number": "16", "publisher": "IOP", "pagerange": "Art. No. 165014", "id_number": "CaltechAUTHORS:20141002-114441991", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20141002-114441991", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d\u02bcEconomia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "PL-Grid Infrastructure" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "Davis and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. 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P." } }, { "id": "Thrane-E", "name": { "family": "Thrane", "given": "E." }, "orcid": "0000-0002-4418-3895" }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "Nissanke-S", "name": { "family": "Nissanke", "given": "S." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } } ] }, "title": "Search for Gravitational Waves Associated with \u03b3-ray Bursts Detected by the Interplanetary Network", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2014 American Physical Society.\n\nReceived 7 April 2014; Published 30 June 2014.\n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory, the\nScience and Technology Facilities Council of the United\nKingdom, the Max Planck Society, and the State of\nNiedersachsen, Germany, for support of the construction\nand operation of the GEO600 detector and the Italian\nIstituto Nazionale di Fisica Nucleare and the French Centre\nNational de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors also\ngratefully acknowledge the support of the research by\nthese agencies and by the Australian Research Council,\nthe International Science Linkages program of the\nCommonwealth of Australia, the Council of Scientific\nand Industrial Research of India, the Istituto Nazionale\ndi Fisica Nucleare of Italy, the Spanish Ministerio de\nEconom\u00eda y Competitividad, the Conselleria d'Economia\nHisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the\nFoundation for Fundamental Research on Matter supported\nby the Netherlands Organisation for Scientific Research,\nthe Polish Ministry of Science and Higher Education,\nthe FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the\nScottish Universities Physics Alliance, The National\nAeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. K. H. acknowledges IPN support from the following sources: NASA NNX06AI36G, NNX08AB84G, NNX08AZ85G, NNX09AV61G, and NNX10AR12G (Suzaku), NASA NNG06GI89G,\nNNX07AJ65G, NNX08AN23G, NNX09AO97G, NNX10AI23G (Swift), NASA NNG06GE69G, NNX07AQ22G, NNX08AC90G, NNX08AX95G,\nNNX09AR28G (INTEGRAL). TheKonus-Wind experiment is partially supported by a Russian Space Agency contract\nand RFBRGrantsNo. 12-02-00032-a and No. 13-02-12017-ofi_m. This document has been assigned LIGO Laboratory document number LIGO-P1300226-v10.\n\nPublished - PhysRevLett.113.011102.pdf
Submitted - 1403.6639v2.pdf
Supplemental Material - Supplementarymaterial_LR14000Aasi.pdf
Supplemental Material - Supplementarymaterial_LR14000Aasi.tex
", "abstract": "We present the results of a search for gravitational waves associated with 223 \u03b3-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005\u20132010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10^(\u22122)M\u2299c^2 at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.", "date": "2014-07-04", "date_type": "published", "publication": "Physical Review Letters", "volume": "113", "number": "1", "publisher": "American Physical Society", "pagerange": "Art. No. 011102", "id_number": "CaltechAUTHORS:20140818-125913710", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140818-125913710", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research of India" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "NASA", "grant_number": "NNX06AI36G" }, { "agency": "NASA", "grant_number": "NNX08AB84G" }, { "agency": "NASA", "grant_number": "NNX08AZ85G" }, { "agency": "NASA", "grant_number": "NNX09AV61G" }, { "agency": "NASA", "grant_number": "NNX10AR12G" }, { "agency": "NASA", "grant_number": "NNG06GI89G" }, { "agency": "NASA", "grant_number": "NNX07AJ65G" }, { "agency": "NASA", "grant_number": "NNX08AN23G" }, { "agency": "NASA", "grant_number": "NNX09AO97G" }, { "agency": "NASA", "grant_number": "NNX10AI23G" }, { "agency": "NASA", "grant_number": "NNG06GE69G" }, { "agency": "NASA", "grant_number": "NNX07AQ22G" }, { "agency": "NASA", "grant_number": "NNX08AC90G" }, { "agency": "NASA", "grant_number": "NNX08AX95G" }, { "agency": "NASA", "grant_number": "NNX09AR28G" }, { "agency": "Russian Foundation for Basic Research", "grant_number": "12-02-00032-a" }, { "agency": "Russian Foundation for Basic Research", "grant_number": "13-02-12017-ofi_m" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Russian Space Agency" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1300226-v10", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration", "IPN Collaboration" ] }, "doi": "10.1103/PhysRevLett.113.011102", "primary_object": { "basename": "1403.6639v2.pdf", "url": "https://authors.library.caltech.edu/records/qzqmn-v1w63/files/1403.6639v2.pdf" }, "related_objects": [ { "basename": "PhysRevLett.113.011102.pdf", "url": "https://authors.library.caltech.edu/records/qzqmn-v1w63/files/PhysRevLett.113.011102.pdf" }, { "basename": "Supplementarymaterial_LR14000Aasi.pdf", "url": "https://authors.library.caltech.edu/records/qzqmn-v1w63/files/Supplementarymaterial_LR14000Aasi.pdf" }, { "basename": "Supplementarymaterial_LR14000Aasi.tex", "url": "https://authors.library.caltech.edu/records/qzqmn-v1w63/files/Supplementarymaterial_LR14000Aasi.tex" } ], "resource_type": "article", "pub_year": "2014", "author_list": "Aasi, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/ms396-1gk06", "eprint_id": 48237, "eprint_status": "archive", "datestamp": "2023-08-20 01:26:52", "lastmod": "2023-10-17 18:38:13", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Abernathy-M-R", "name": { "family": "Abernathy", "given": "M. R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-R-A", "name": { "family": "Anderson", "given": "R. A." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. 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Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D. B." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lewis-J", "name": { "family": "Lewis", "given": "J." } }, { "id": "Li-T-G-F", "name": { "family": "Li", "given": "T. G. F." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Martynov-D", "name": { "family": "Martynov", "given": "D." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Phelps-M", "name": { "family": "Phelps", "given": "M." } }, { "id": "Price-L-R", "name": { "family": "Price", "given": "L. R." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Quintero-E-A", "name": { "family": "Quintero", "given": "E." } }, { "id": "Raymond-V", "name": { "family": "Raymond", "given": "V." } }, { "id": "Rollins-J-G", "name": { "family": "Rollins", "given": "J. G." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Shao-Z", "name": { "family": "Shao", "given": "Z." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Singer-L", "name": { "family": "Singer", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Smith-R-J-E", "name": { "family": "Smith", "given": "R. J. E." } }, { "id": "Smith-Lefebvre-N-D", "name": { "family": "Smith-Lefebvre", "given": "N. D." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Thrane-E", "name": { "family": "Thrane", "given": "E." }, "orcid": "0000-0002-4418-3895" }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "Nissanke-S", "name": { "family": "Nissanke", "given": "S." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } } ] }, "title": "Methods and results of a search for gravitational waves associated with gamma-ray bursts using the GEO 600, LIGO, and Virgo detectors", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2014 American Physical Society.\n\nReceived 23 May 2014; Published 25 June 2014.\n\nWe are indebted to the observers of the electromagnetic\nevents and the Gamma-ray burst Coordinates Network for\nproviding us with valuable data. The authors gratefully\nacknowledge the support of the United States National\nScience Foundation for the construction and operation of\nthe LIGO Laboratory, the Science and Technology\nFacilities Council of the United Kingdom, the Max-\nPlanck-Society, and the State of Niedersachsen/Germany\nfor support of the construction and operation of the GEO\n600 detector, and the Italian Istituto Nazionale di Fisica\nNucleare and the French Centre National de la Recherche\nScientifique for the construction and operation of the Virgo\ndetector. The authors also gratefully acknowledge the\nsupport of the research by these agencies and by the\nAustralian Research Council, the International Science\nLinkages program of the Commonwealth of Australia,\nthe Council of Scientific and Industrial Research of\nIndia, the Istituto Nazionale di Fisica Nucleare of Italy,\nthe Spanish Ministerio de Econom\u00eda y Competitividad, the\nConselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern\nde les Illes Balears, the Foundation for Fundamental\nResearch on Matter supported by the Netherlands\nOrganisation for Scientific Research, the Polish Ministry\nof Science and Higher Education, the FOCUS Programme\nof Foundation for Polish Science, the Royal Society, the\nScottish Funding Council, the Scottish Universities Physics\nAlliance, the National Aeronautics and Space\nAdministration, the National Research Foundation of\nKorea, Industry Canada and the Province of Ontario\nthrough the Ministry of Economic Development and\nInnovation, the National Science and Engineering\nResearch Council Canada, the Carnegie Trust, the\nLeverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation, and the Alfred P.\nSloan Foundation. We also gratefully acknowledge the\nteam of graduate students and scientists who maintained the\nH2 instrument during the Astrowatch epoch, without whom\na substantial fraction of our events would not have been\nanalyzed. This paper has been assigned LIGO Document\nNo. LIGO-P1300086.\n\nPublished - PhysRevD.89.122004.pdf
Submitted - 1405.1053v2.pdf
", "abstract": "In this paper we report on a search for short-duration gravitational wave bursts in the frequency range 64 Hz\u20131792 Hz associated with gamma-ray bursts (GRBs), using data from GEO 600 and one of the LIGO or Virgo detectors. We introduce the method of a linear search grid to analyze GRB events with large sky localization uncertainties, for example the localizations provided by the Fermi Gamma-ray Burst Monitor (GBM). Coherent searches for gravitational waves (GWs) can be computationally intensive when the GRB sky position is not well localized, due to the corrections required for the difference in arrival time between detectors. Using a linear search grid we are able to reduce the computational cost of the analysis by a factor of O(10) for GBM events. Furthermore, we demonstrate that our analysis pipeline can improve upon the sky localization of GRBs detected by the GBM, if a high-frequency GW signal is observed in coincidence. We use the method of the linear grid in a search for GWs associated with 129 GRBs observed satellite-based gamma-ray experiments between 2006 and 2011. The GRBs in our sample had not been previously analyzed for GW counterparts. A fraction of our GRB events are analyzed using data from GEO 600 while the detector was using squeezed-light states to improve its sensitivity; this is the first search for GWs using data from a squeezed-light interferometric observatory. We find no evidence for GW signals, either with any individual GRB in this sample or with the population as a whole. For each GRB we place lower bounds on the distance to the progenitor, under an assumption of a fixed GW emission energy of 10^(\u22122)M\u2299c^2, with a median exclusion distance of 0.8 Mpc for emission at 500 Hz and 0.3 Mpc at 1 kHz. The reduced computational cost associated with a linear search grid will enable rapid searches for GWs associated with Fermi GBM events once the advanced LIGO and Virgo detectors begin operation.", "date": "2014-06-15", "date_type": "published", "publication": "Physical Review D", "volume": "89", "number": "12", "publisher": "American Physical Society", "pagerange": "Art. No. 122004", "id_number": "CaltechAUTHORS:20140808-100111073", "issn": "1550-7998", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140808-100111073", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Science and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ontario Ministry of Research and Innovation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1300086", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "TAPIR" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.89.122004", "primary_object": { "basename": "1405.1053v2.pdf", "url": "https://authors.library.caltech.edu/records/ms396-1gk06/files/1405.1053v2.pdf" }, "related_objects": [ { "basename": "PhysRevD.89.122004.pdf", "url": "https://authors.library.caltech.edu/records/ms396-1gk06/files/PhysRevD.89.122004.pdf" } ], "resource_type": "article", "pub_year": "2014", "author_list": "Aasi, J.; Abbott, B. 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I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Santamar\u00eda-L", "name": { "family": "Santamar\u00eda", "given": "L." } }, { "id": "Sperhake-U", "name": { "family": "Sperhake", "given": "U." }, "orcid": "0000-0002-3134-7088" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "M\u00f6sta-P", "name": { "family": "Moesta", "given": "P." }, "orcid": "0000-0002-9371-1447" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Buchman-L-T", "name": { "family": "Buchman", "given": "L. T." } }, { "id": "Reisswig-C", "name": { "family": "Reisswig", "given": "C." } }, { "id": "Scheel-M-A", "name": { "family": "Scheel", "given": "M. A." } }, { "id": "Szil\u00e1gyi-B", "name": { "family": "Szil\u00e1gyi", "given": "B." } }, { "id": "Taylor-N-W", "name": { "family": "Taylor", "given": "N. W." } } ] }, "title": "The NINJA-2 project: detecting and characterizing gravitational waveforms modelled using numerical binary black hole simulations", "ispublished": "pub", "full_text_status": "public", "keywords": "numerical relativity, gravitational-wave astronomy, binary black holes, NINJA, LIGO, Virgo", "note": "\u00a9 2014 Institute of Physics. \n\nReceived 14 January 2014, revised 27 March 2014. Accepted for publication 11 April 2014. Published 20 May 2014. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the\nCommonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and\nSpace Administration, OTKA of Hungary, the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P Sloan Foundation. We gratefully acknowledge support from the National Science Foundation under NSF\ngrants PHY-1305730, PHY-1212426, PHY-1229173, AST-1028087, DRL-1136221, OCI-0832606, PHY-0903782, PHY-0929114, PHY-0969855, AST-1002667, PHY-0963136, PHY-1300903, PHY-1305387, PHY-1204334, PHY-0855315, PHY-0969111, PHY-1005426, PHY-0601459, PHY-1068881, PHY-1005655, PHY-0653443, PHY-0855892, PHY-0914553, PHY-0941417, PHY-0903973, PHY-0955825, by NASA grants 07-ATFP07-0158, NNX11AE11G, NNX13AH44G, NNX09AF96G, NNX09AF97G, by Marie Curie Grants of the 7th European Community Framework Programme FP7-PEOPLE-2011-CIG CBHEO No. 293412, by the\nDyBHo-256667 ERC Starting Grant, and MIRG-CT-2007-205005/PHY, and Science and Technology Facilities Council grants ST/H008438/1 and ST/I001085/1. Further funding was provided by the Sherman Fairchild Foundation, NSERC of Canada, the Canada Research Chairs Program, the Canadian Institute for Advanced Research, the Ram\u03ccn y\nCajal Programme of the Ministry of Education and Science of Spain, contracts AYA2010-15709, CSD2007-00042, CSD2009-00064 and FPA2010-16495 of the Spanish Ministry\nof Science and Innovation, the German Research Foundation, grant SFB/Transregio 7, the German Aerospace Center for LISA Germany, and the Grand-in-Aid for Scientific Research (24103006). Computations were carried out on Teragrid machines Lonestar, Ranger, Trestles and Kraken under Teragrid allocations TG-PHY060027N, TG-MCA99S008,\nTG-PHY090095, TG-PHY100051, TG-PHY990007N, TG-PHY090003, TG-MCA08X009. Computations were also performed on the clusters \"HLRB-2' at LRZ Munich, 'NewHorizons' and 'Blue Sky' at RIT (funded by NSF grant nos PHY-1229173, AST-1028087, DMS-0820923 and PHY-0722703), 'Zwicky' at Caltech (funded by NSF MRI award PHY-0960291), 'Finis\nTerrae' (funded by CESGA-ICTS-2010-200), 'Caesaraugusta' (funded by BSC grant nos AECT-2011-2-0006, AECT-2011-3-0007), 'MareNostrum' (funded by BSC grant nos. AECT-2009-2-0017, AECT-2010-1-0008, AECT-2010-2-0013, AECT-2010-3-0010, AECT-2011-1-0015, AECT-2011-2-0012), 'VSC' in Vienna (funded by FWF grant P22498), 'Force' at\nGaTech, and on the GPC supercomputer at the SciNet HPC Consortium [150]; SciNet is funded by: the Canada Foundation for Innovation under the auspices of Compute Canada; the Government of Ontario; Ontario Research Fund\u2014Research Excellence; and the University of Toronto.\n\nSubmitted - 1401.0939v1.pdf
", "abstract": "The Numerical INJection Analysis (NINJA) project is a collaborative effort between members of the numerical relativity and gravitational-wave (GW) astrophysics communities. The purpose of NINJA is to study the ability to detect GWs emitted from merging binary black holes (BBH) and recover their parameters with next-generation GW observatories. We report here on the results of the second NINJA project, NINJA-2, which employs 60 complete BBH hybrid waveforms consisting of a numerical portion modelling the late inspiral, merger, and ringdown stitched to a post-Newtonian portion modelling the early inspiral. In a 'blind injection challenge' similar to that conducted in recent Laser Interferometer Gravitational Wave Observatory (LIGO) and Virgo science runs, we added seven hybrid waveforms to two months of data recoloured to predictions of Advanced LIGO (aLIGO) and Advanced Virgo (AdV) sensitivity curves during their first observing runs. The resulting data was analysed by GW detection algorithms and 6 of the waveforms were recovered with false alarm rates smaller than 1 in a thousand years. Parameter-estimation algorithms were run on each of these waveforms to explore the ability to constrain the masses, component angular momenta and sky position of these waveforms. We find that the strong degeneracy between the mass ratio and the BHs' angular momenta will make it difficult to precisely estimate these parameters with aLIGO and AdV. We also perform a large-scale Monte Carlo study to assess the ability to recover each of the 60 hybrid waveforms with early aLIGO and AdV sensitivity curves. Our results predict that early aLIGO and AdV will have a volume-weighted average sensitive distance of 300 Mpc (1 Gpc) for 10M_\u2299 + 10M_\u2299 (50M_\u2299 + 50M_\u2299) BBH coalescences. We demonstrate that neglecting the component angular momenta in the waveform models used in matched-filtering will result in a reduction in sensitivity for systems with large component angular momenta. This reduction is estimated to be up to ~15% for 50M_\u2299 + 50M_\u2299 BBH coalescences with almost maximal angular momenta aligned with the orbit when using early aLIGO and AdV sensitivity curves.", "date": "2014-06-07", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "31", "number": "11", "publisher": "IOP", "pagerange": "Art. No. 115004", "id_number": "CaltechAUTHORS:20140626-115501423", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140626-115501423", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Australian Research Council" }, { "agency": "Commonwealth of Australia International Science Linkages Program" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. 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I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "M\u00f6sta-P", "name": { "family": "Moesta", "given": "P." }, "orcid": "0000-0002-9371-1447" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Reitze-D-H", "name": { "family": "Reitze", "given": "D. H." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } } ] }, "title": "Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005\u20132010", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2014 American Physical Society. \n\nReceived 28 March 2014; published 27 May 2014. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u00f3n y Ciencia, the Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucille Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - PhysRevD.89.102006.pdf
Submitted - 1403.5306v2.pdf
", "abstract": "We report results from a search for gravitational waves produced by perturbed intermediate mass black holes (IMBH) in data collected by LIGO and Virgo between 2005 and 2010. The search was sensitive to astrophysical sources that produced damped sinusoid gravitational wave signals, also known as ringdowns, with frequency 50\u2264f_0/Hz\u22642000 and decay timescale 0.0001\u2272\u03c4/s\u22720.1 characteristic of those produced in mergers of IMBH pairs. No significant gravitational wave candidate was detected. We report upper limits on the astrophysical coalescence rates of IMBHs with total binary mass 50\u2264M/M_\u2299\u2264450 and component mass ratios of either 1:1 or 4:1. For systems with total mass 100\u2264M/M_\u2299\u2264150, we report a 90% confidence upper limit on the rate of binary IMBH mergers with nonspinning and equal mass components of 6.9\u00d710^(\u22128)\u2009\u2009Mpc^(\u22123)\u2009yr^(\u22121). We also report a rate upper limit for ringdown waveforms from perturbed IMBHs, radiating 1% of their mass as gravitational waves in the fundamental, \u2113=m=2, oscillation mode, that is nearly three orders of magnitude more stringent than previous results.", "date": "2014-05-15", "date_type": "published", "publication": "Physical Review D", "volume": "89", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102006", "id_number": "CaltechAUTHORS:20140630-140920794", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140630-140920794", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Australian Research Council" }, { "agency": "Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.89.102006", "primary_object": { "basename": "1403.5306v2.pdf", "url": "https://authors.library.caltech.edu/records/brsdq-1t853/files/1403.5306v2.pdf" }, "related_objects": [ { "basename": "PhysRevD.89.102006.pdf", "url": "https://authors.library.caltech.edu/records/brsdq-1t853/files/PhysRevD.89.102006.pdf" } ], "resource_type": "article", "pub_year": "2014", "author_list": "Aasi, J.; Abbott, B. 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D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } } ] }, "title": "Application of a Hough search for continuous gravitational waves on data from the fifth LIGO science run", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves, LIGO, neutron stars", "note": "\u00a9 2014 Institute of Physics. Received 28 November 2013, revised 18 February 2014. Accepted for publication 7 March 2014. Published 3 April 2014. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The\nauthors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the\nCommonwealth of Australia, the Council of Scientific and Industrial Research of India,\nthe Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y\nCompetitividad, the Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes\nBalears, the Foundation for Fundamental Research on Matter supported by the Netherlands\nOrganisation for Scientific Research, the Polish Ministry of Science and Higher Education,\nthe FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish\nFunding Council, the Scottish Universities Physics Alliance, The National Aeronautics and\nSpace Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation, and the Alfred P Sloan Foundation. This document has\nbeen assigned LIGO Laboratory document number LIGO-P1300071.\n\nSubmitted - 1311.2409v3.pdf
", "abstract": "We report on an all-sky search for periodic gravitational waves in the frequency range 50\u20131000\u2009Hz with the first derivative of frequency in the range \u22128.9 \u00d7 10^(\u221210) Hz\u2009s^(\u22121) to zero in two years of data collected during LIGO's fifth science run. Our results employ a Hough transform technique, introducing a \u03c7^2 test and analysis of coincidences between the signal levels in years 1 and 2 of observations that offers a significant improvement in the product of strain sensitivity with compute cycles per data sample compared to previously published searches. Since our search yields no surviving candidates, we present results taking the form of frequency dependent, 95% confidence upper limits on the strain amplitude h0. The most stringent upper limit from year 1 is 1.0 \u00d7 10^(\u221224) in the 158.00\u2013158.25\u2009Hz band. In year 2, the most stringent upper limit is 8.9 \u00d7 10^(\u221225) in the 146.50\u2013146.75\u2009Hz band. This improved detection pipeline, which is computationally efficient by at least two orders of magnitude better than our flagship Einstein@Home search, will be important for 'quick-look' searches in the Advanced LIGO and Virgo detector era.", "date": "2014-04-21", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "31", "number": "8", "publisher": "IOP", "pagerange": "Art. No. 085014", "id_number": "CaltechAUTHORS:20140603-092556549", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140603-092556549", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (UK)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research of India" }, { "agency": "Istituto Nazionale di Fisica Nucleare of Italy" }, { "agency": "Spanish Ministerio de Econom\u00eda y Competitividad" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research" }, { "agency": "Polish Ministry of Science and Higher Education" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "P1300071", "name": "LIGO Laboratory document number" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1088/0264-9381/31/8/085014", "primary_object": { "basename": "1311.2409v3.pdf", "url": "https://authors.library.caltech.edu/records/dyaya-fck89/files/1311.2409v3.pdf" }, "resource_type": "article", "pub_year": "2014", "author_list": "Aasi, J.; Abadie, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/q49gz-5fw52", "eprint_id": 41552, "eprint_status": "archive", "datestamp": "2023-08-20 00:26:33", "lastmod": "2023-10-24 23:50:07", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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E." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Hong-T", "name": { "family": "Hong", "given": "T." } }, { "id": "Kaufman-K", "name": { "family": "Kaufman", "given": "K." } }, { "id": "Luan-Jing", "name": { "family": "Luan", "given": "J." }, "orcid": "0000-0001-6048-1959" }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } } ] }, "title": "Gravitational-waves from known pulsars: results from the initial detector era", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational-waves - pulsars: general", "note": "\u00a9 2014 American Astronomical Society. Received 2013 September 30; accepted 2014 February 28; published 2014 April 2. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, the National Aeronautics and Space Administration, OTKA of Hungary, the Lyon Institute of Origins (LIO), the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. The Nan\u00e7ay Radio Observatory is operated by the Paris Observatory, associated with the French Centre National de la Recherche Scientifique. LIGO Document No. LIGO-P1200104.\n\nPublished - Aasi_2014_ApJ_785_119.pdf
Submitted - 1309.4027.pdf
", "abstract": "We present the results of searches for gravitational waves from a large selection of pulsars using data from the most recent science runs (S6, VSR2 and VSR4) of the initial generation of interferometric gravitational wave detectors LIGO (Laser Interferometric Gravitational-wave Observatory) and Virgo. We do not see evidence for gravitational wave emission from any of the targeted sources but produce upper limits on the emission amplitude. We highlight the results from seven young pulsars with large spin-down luminosities. We reach within a factor of five of the canonical spin-down limit for all seven of these, whilst for the Crab and Vela pulsars we further surpass their spin-down limits. We present new or updated limits for 172 other pulsars (including both young and millisecond pulsars). Now that the detectors are undergoing major upgrades, and, for completeness, we bring together all of the most up-to-date results from all pulsars searched for during the operations of the first-generation LIGO, Virgo and GEO600 detectors. This gives a total of 195 pulsars including the most recent results described in this paper.", "date": "2014-04-20", "date_type": "published", "publication": "Astrophysical Journal", "volume": "785", "number": "2", "publisher": "American Astronomical Society", "pagerange": "Art. No. 119", "id_number": "CaltechAUTHORS:20130930-103904702", "issn": "0004-637X", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130930-103904702", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Research and Innovation" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1200104", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1088/0004-637X/785/2/119", "primary_object": { "basename": "1309.4027.pdf", "url": "https://authors.library.caltech.edu/records/q49gz-5fw52/files/1309.4027.pdf" }, "related_objects": [ { "basename": "Aasi_2014_ApJ_785_119.pdf", "url": "https://authors.library.caltech.edu/records/q49gz-5fw52/files/Aasi_2014_ApJ_785_119.pdf" } ], "resource_type": "article", "pub_year": "2014", "author_list": "Aasi, J.; Abadie, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/q3py1-z5n73", "eprint_id": 44724, "eprint_status": "archive", "datestamp": "2023-08-22 11:50:15", "lastmod": "2023-10-26 14:54:27", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Abernathy-M-R", "name": { "family": "Abernathy", "given": "M. R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-R-A", "name": { "family": "Anderson", "given": "R. A." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Austin-L", "name": { "family": "Austin", "given": "L." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chakraborty-R", "name": { "family": "Chakraborty", "given": "R." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Daudert-B", "name": { "family": "Daudert", "given": "B." } }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "Driggers-J-C", "name": { "family": "Driggers", "given": "J. C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Fotopoulos-N", "name": { "family": "Fotopoulos", "given": "N." } }, { "id": "Gushwa-K-E", "name": { "family": "Gushwa", "given": "K. E." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hall-E", "name": { "family": "Hall", "given": "E." } }, { "id": "Harms-J", "name": { "family": "Harms", "given": "J." }, "orcid": "0000-0002-7332-9806" }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Lewis-J-B", "name": { "family": "Lewis", "given": "J. B." } }, { "id": "Litvine-V", "name": { "family": "Litvine", "given": "V." } }, { "id": "Lloyd-D", "name": { "family": "Lloyd", "given": "D." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Martynov-D", "name": { "family": "Martynov", "given": "D." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Phelps-M", "name": { "family": "Phelps", "given": "M." } }, { "id": "Poux-C", "name": { "family": "Poux", "given": "C." } }, { "id": "Price-L-R", "name": { "family": "Price", "given": "L. R." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Quintero-E-A", "name": { "family": "Quintero", "given": "E." } }, { "id": "Raymond-V", "name": { "family": "Raymond", "given": "V." } }, { "id": "Reitze-D-H", "name": { "family": "Reitze", "given": "D. H." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Rollins-J-G", "name": { "family": "Rollins", "given": "J. G." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Singer-L", "name": { "family": "Singer", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Smith-Lefebvre-N-D", "name": { "family": "Smith-Lefebvre", "given": "N. D." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Thrane-E", "name": { "family": "Thrane", "given": "E." }, "orcid": "0000-0002-4418-3895" }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Hong-T", "name": { "family": "Hong", "given": "T." } }, { "id": "Kaufman-K", "name": { "family": "Kaufman", "given": "K." } }, { "id": "Luan-Jing", "name": { "family": "Luan", "given": "J." }, "orcid": "0000-0001-6048-1959" }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Cao-Yi", "name": { "family": "Cao", "given": "Y." }, "orcid": "0000-0002-8036-8491" }, { "id": "Laher-R-R", "name": { "family": "Laher", "given": "R. R." }, "orcid": "0000-0003-2451-5482" }, { "id": "Nissanke-S", "name": { "family": "Nissanke", "given": "S." } }, { "id": "Heptonstall-A-W", "name": { "family": "Heptonstall", "given": "A. W." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Jacobson-M", "name": { "family": "Jacobson", "given": "M." } }, { "id": "James-E", "name": { "family": "James", "given": "E." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Korth-W-Z", "name": { "family": "Korth", "given": "W. Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Kasliwal-M-M", "name": { "family": "Kasliwal", "given": "M. M." }, "orcid": "0000-0002-5619-4938" } ] }, "title": "First Searches for Optical Counterparts to Gravitational-Wave Candidate Events", "ispublished": "pub", "full_text_status": "public", "keywords": "binaries: close; catalogs; gravitational waves; stars: neutron; surveys", "note": "\u00a9 2014 American Astronomical Society. Received 2013 October 30; accepted 2014 January 18; published 2014 February 11. We thank J. Barnes, D. Kasen, B. Metzger, and E. Nakar for\nproviding the kilonova model light curves that we have used in our Figures 4\u20137. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully\nacknowledge the support of the research by these agencies\nand by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Economia y Competitividad, the Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, OTKA of Hungary, the Lyon Institute of Origins (LIO), the National\nResearch Foundation of Korea, Industry Canada and the\nProvince of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, FIRB 2012 Project RBFR12PM1F (Italian Ministry of Education, University and Research), and the Alfred P. Sloan Foundation. This work is based on results partially obtained at the ESO observatory, La Silla. The Liverpool Telescope is operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council. This document has been assigned the identifier LIGO-P1200171-v19.\n\nPublished - 0067-0049_211_1_7.pdf
Submitted - 1310.2314v2.pdf
", "abstract": "During the Laser Interferometer Gravitational-wave Observatory and Virgo joint science runs in 2009-2010, gravitational wave (GW) data from three interferometer detectors were analyzed within minutes to select GW candidate events and infer their apparent sky positions. Target coordinates were transmitted to several telescopes for follow-up observations aimed at the detection of an associated optical transient. Images were obtained for eight such GW candidates. We present the methods used to analyze the image data as well as the transient search results. No optical transient was identified with a convincing association with any of these candidates, and none of the GW triggers showed strong evidence for being astrophysical in nature. We compare the sensitivities of these observations to several model light curves from possible sources of interest, and discuss prospects for future joint GW-optical observations of this type.", "date": "2014-03", "date_type": "published", "publication": "Astrophysical Journal Supplement Series", "volume": "211", "number": "1", "publisher": "American Astronomical Society", "pagerange": "Art. No. 7", "id_number": "CaltechAUTHORS:20140408-071345962", "issn": "0067-0049", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140408-071345962", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears" }, { "agency": "Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "FIRB 2012 Project", "grant_number": "RBFR12PM1F" }, { "agency": "Ministero dell'Istruzione, dell'Universit\u00e0 e della Ricerca (MIUR)" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Ontario Ministry of Economic Development and Innovation" } ] }, "other_numbering_system": { "items": [ { "id": "P1200171-v19", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" }, { "id": "Palomar-Transient-Factory" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1088/0067-0049/211/1/7", "primary_object": { "basename": "0067-0049_211_1_7.pdf", "url": "https://authors.library.caltech.edu/records/q3py1-z5n73/files/0067-0049_211_1_7.pdf" }, "related_objects": [ { "basename": "1310.2314v2.pdf", "url": "https://authors.library.caltech.edu/records/q3py1-z5n73/files/1310.2314v2.pdf" } ], "resource_type": "article", "pub_year": "2014", "author_list": "Aasi, J.; Abadie, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/phb2k-tbn07", "eprint_id": 44609, "eprint_status": "archive", "datestamp": "2023-08-19 23:32:29", "lastmod": "2023-10-26 14:49:06", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "Curt" } }, { "id": "Burke-Spolaor-S", "name": { "family": "Burke-Spolaor", "given": "Sarah" }, "orcid": "0000-0003-4052-7838" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" }, { "id": "Lazio-J-W", "name": { "family": "Lazio", "given": "Joseph" } }, { "id": "Majid-W-A", "name": { "family": "Majid", "given": "Walid" }, "orcid": "0000-0002-4694-4221" } ] }, "title": "The gravitational-wave discovery space of pulsar timing arrays", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2014 American Physical Society. Received 11 September 2013; published 18 February 2014. C. C. gratefully acknowledges support from NSF Grant No. PHY-1068881. M. V. is grateful for support from the JPL RTD program. This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract to the National Aeronautics and Space Administration.\n\nPublished - PhysRevD.89.042003.pdf
Submitted - 1309.2581v1.pdf
", "abstract": "Recent years have seen a burgeoning interest in using pulsar timing arrays (PTAs) as gravitational-wave (GW) detectors. To date, that interest has focused mainly on three particularly promising source types: supermassive black hole binaries, cosmic strings, and the stochastic background from early-Universe phase transitions. In this paper, by contrast, our aim is to investigate the PTA potential for discovering unanticipated sources. We derive significant constraints on the available discovery space based solely on energetic and statistical considerations: we show that a PTA detection of GWs at frequencies above \u223c10^(\u22125)\u2009\u2009Hz would either be an extraordinary coincidence or violate \"cherished beliefs;\" we show that for PTAs GW memory can be more detectable than direct GWs, and that, as we consider events at ever higher redshift, the memory effect increasingly dominates an event's total signal-to-noise ratio. The paper includes also a simple analysis of the effects of pulsar red noise in PTA searches, and a demonstration that the effects of periodic GWs in the \u223c10^(\u22127)\u201310^(\u22124.5)\u2009\u2009Hz band would not be degenerate with small errors in standard pulsar parameters (except in a few narrow bands).", "date": "2014-02-18", "date_type": "published", "publication": "Physical Review D", "volume": "89", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 042003", "id_number": "CaltechAUTHORS:20140402-133231801", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140402-133231801", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "PHY-1068881" }, { "agency": "JPL Research and Technology Development Fund" }, { "agency": "NASA/JPL/Caltech" } ] }, "doi": "10.1103/PhysRevD.89.042003", "primary_object": { "basename": "1309.2581v1.pdf", "url": "https://authors.library.caltech.edu/records/phb2k-tbn07/files/1309.2581v1.pdf" }, "related_objects": [ { "basename": "PhysRevD.89.042003.pdf", "url": "https://authors.library.caltech.edu/records/phb2k-tbn07/files/PhysRevD.89.042003.pdf" } ], "resource_type": "article", "pub_year": "2014", "author_list": "Cutler, Curt; Burke-Spolaor, Sarah; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/vs8ym-ep930", "eprint_id": 43573, "eprint_status": "archive", "datestamp": "2023-08-19 22:35:46", "lastmod": "2023-10-25 23:40:35", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Abernathy-M-R", "name": { "family": "Abernathy", "given": "M. R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R. X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-R-A", "name": { "family": "Anderson", "given": "R. A." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Austin-L", "name": { "family": "Austin", "given": "L." } }, { "id": "Barayoga-J-C", "name": { "family": "Barayoga", "given": "J. C." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chakraborty-R", "name": { "family": "Chakraborty", "given": "R." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Daudert-B", "name": { "family": "Daudert", "given": "B." } }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Driggers-J-C", "name": { "family": "Driggers", "given": "J. C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Fotopoulos-N", "name": { "family": "Fotopoulos", "given": "N." } }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Gushwa-K-E", "name": { "family": "Gushwa", "given": "K. E." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hall-E", "name": { "family": "Hall", "given": "E." } }, { "id": "Harms-J", "name": { "family": "Harms", "given": "J." }, "orcid": "0000-0002-7332-9806" }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A-W", "name": { "family": "Heptonstall", "given": "A. W." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Hong-T", "name": { "family": "Hong", "given": "T." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Jacobson-M", "name": { "family": "Jacobson", "given": "M." } }, { "id": "James-E", "name": { "family": "James", "given": "E." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kaufman-K", "name": { "family": "Kaufman", "given": "K." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Korth-W-Z", "name": { "family": "Korth", "given": "W. Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lewis-J-B", "name": { "family": "Lewis", "given": "J. B." } }, { "id": "Lloyd-D", "name": { "family": "Lloyd", "given": "D." } }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Martynov-D", "name": { "family": "Martynov", "given": "D." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Phelps-M", "name": { "family": "Phelps", "given": "M." } }, { "id": "Poux-C", "name": { "family": "Poux", "given": "C." } }, { "id": "Price-L-R", "name": { "family": "Price", "given": "L. R." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Quintero-E-A", "name": { "family": "Quintero", "given": "E." } }, { "id": "Raymond-V", "name": { "family": "Raymond", "given": "V." } }, { "id": "Rollins-J-G", "name": { "family": "Rollins", "given": "J. G." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Singer-L", "name": { "family": "Singer", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Smith-Lefebvre-N-D", "name": { "family": "Smith-Lefebvre", "given": "N. D." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thirugnanasambandam-M-P", "name": { "family": "Thirugnanasambandam", "given": "M. P." } }, { "id": "Thrane-E", "name": { "family": "Thrane", "given": "E." }, "orcid": "0000-0002-4418-3895" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } } ] }, "title": "Search for long-lived gravitational-wave transients coincident with long gamma-ray bursts", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2013 American Physical Society.\n\nReceived 9 October 2013; published 13 December 2013.\n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory, the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre\nNational de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors also\ngratefully acknowledge the support of the research by\nthese agencies and by the Australian Research Council,\nthe International Science Linkages program of the\nCommonwealth of Australia, the Council of Scientific\nand Industrial Research of India, the Istituto Nazionale di\nFisica Nucleare of Italy, the Spanish Ministerio de\nEconom\u0131\u00b4a y Competitividad, the Conselleria d'Economia\nHisenda i Innovacio\u00b4 of the Govern de les Illes Balears, the\nFoundation for Fundamental Research on Matter supported\nby the Netherlands Organisation for Scientific Research,\nthe Polish Ministry of Science and Higher Education, the\nFOCUS Programme of Foundation for Polish Science, the\nRoyal Society, the Scottish Funding Council, the Scottish\nUniversities Physics Alliance, The National Aeronautics\nand Space Administration, OTKA of Hungary, the Lyon\nInstitute of Origins (LIO), the National Research\nFoundation of Korea, Industry Canada and the Province\nof Ontario through the Ministry of Economic Development\nand Innovation, the National Science and Engineering\nResearch Council Canada, the Carnegie Trust, the\nLeverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation, and the Alfred P.\nSloan Foundation.\n\nPublished - PhysRevD.88.122004.pdf
Submitted - 1309.6160v3.pdf
", "abstract": "Long gamma-ray bursts (GRBs) have been linked to extreme core-collapse supernovae from massivestars. Gravitational waves (GW) offer a probe of the physics behind long GRBs. We investigate models of long-lived (~10\u20131000 s) GW emission associated with the accretion disk of a collapsed star or with its\nprotoneutron star remnant. Using data from LIGO's fifth science run, and GRB triggers from the Swift experiment, we perform a search for unmodeled long-lived GW transients. Finding no evidence of GW emission, we place 90% confidence-level upper limits on the GW fluence at Earth from long GRBs for\nthree waveforms inspired by a model of GWs from accretion disk instabilities. These limits range from F < 3:5 ergs cm^(-2) to F < 1200 ergs cm^(-2), depending on the GRB and on the model, allowing us to probe\noptimistic scenarios of GW production out to distances as far as \u2248 33 Mpc. Advanced detectors are expected to achieve strain sensitivities 10x better than initial LIGO, potentially allowing us to probe the engines of the nearest long GRBs.", "date": "2013-12-13", "date_type": "published", "publication": "Physical Review D", "volume": "88", "number": "12", "publisher": "American Physical Society", "pagerange": "Article No. 122004", "id_number": "CaltechAUTHORS:20140130-095945569", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140130-095945569", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "LIGO Laboratory" }, { "agency": "Science and Technology Facilities Council (STFC) (UK)" }, { "agency": "Max-Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Italian Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS) (France)" }, { "agency": "Australian Research Council (ARC)" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research of India" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN) (Italy)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (Spain)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Foundation for Fundamental Research on Matter (The Netherlands)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council (SFC)" }, { "agency": "Scottish Universities Physics Alliance (SUPA)" }, { "agency": "NASA" }, { "agency": "OTKA (Hungary)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation (NRF) (Korea)" }, { "agency": "Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation" }, { "agency": "National Science and Engineering Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust (UK)" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.88.122004", "primary_object": { "basename": "1309.6160v3.pdf", "url": "https://authors.library.caltech.edu/records/vs8ym-ep930/files/1309.6160v3.pdf" }, "related_objects": [ { "basename": "PhysRevD.88.122004.pdf", "url": "https://authors.library.caltech.edu/records/vs8ym-ep930/files/PhysRevD.88.122004.pdf" } ], "resource_type": "article", "pub_year": "2013", "author_list": "Aasi, J.; Abadie, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/1njvv-5tf49", "eprint_id": 43510, "eprint_status": "archive", "datestamp": "2023-08-19 22:16:48", "lastmod": "2023-10-25 23:36:51", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Aasi-J", "name": { "family": "Aasi", "given": "J." } }, { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Abernathy-M-R", "name": { "family": "Abernathy", "given": "M. 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P." } } ] }, "title": "Directed search for continuous gravitational waves from the Galactic center", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2013 American Physical Society.\nReceived 27 September 2013; published 18 November 2013.\n\n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction and operation of the LIGO Laboratory, the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de\nEconom\u00eda y Competitividad, the Conselleria d'Economia\nHisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the\nFoundation for Fundamental Research on Matter supported\nby the Netherlands Organisation for Scientific Research,\nthe Polish Ministry of Science and Higher Education, the\nFOCUS Programme of Foundation for Polish Science, the\nRoyal Society, the Scottish Funding Council, the Scottish\nUniversities Physics Alliance, The National Aeronautics\nand Space Administration, OTKA of Hungary, the Lyon\nInstitute of Origins (LIO), the National Research\nFoundation of Korea, Industry Canada and the Province\nof Ontario through the Ministry of Economic Development\nand Innovation, the National Science and Engineering\nResearch Council Canada, the Carnegie Trust, the\nLeverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation, and the Alfred P.\nSloan Foundation. This document has been assigned LIGO\nLaboratory Document No. LIGO-P1300037.\n\nPublished - PhysRevD.88.102002.pdf
Submitted - 1309.6221v2.pdf
", "abstract": "We present the results of a directed search for continuous gravitational waves from unknown, isolated neutron stars in the Galactic center region, performed on two years of data from LIGO's fifth science run from two LIGO detectors. The search uses a semicoherent approach, analyzing coherently 630 segments, each spanning 11.5 hours, and then incoherently combining the results of the single segments. It covers gravitational wave frequencies in a range from 78 to 496 Hz and a frequency-dependent range of first-order spindown values down to \u22127.86\u00d710^(\u22128)\u2009\u2009Hz/s at the highest frequency. No gravitational waves were detected. The 90% confidence upper limits on the gravitational wave amplitude of sources at the Galactic center are \u223c3.35\u00d710^(\u221225) for frequencies near 150 Hz. These upper limits are the most constraining to date for a large-parameter-space search for continuous gravitational wave signals.", "date": "2013-11-18", "date_type": "published", "publication": "Physical Review D", "volume": "88", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102002", "id_number": "CaltechAUTHORS:20140124-110416768", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140124-110416768", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Commonwealth of Australia International Science Linkages" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Hungarian Scientific Research Fund (OTKA)" }, { "agency": "Lyon Institute of Origins (LIO)" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. 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A." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Williams-T", "name": { "family": "Williams", "given": "T." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y," }, "orcid": "0000-0002-9730-9463" }, { "id": "Gossan-S", "name": { "family": "Gossan", "given": "S." } }, { "id": "Hong-T", "name": { "family": "Hong", "given": "T." } }, { "id": "Miao-Haixing", "name": { "family": "Miao", "given": "H." }, "orcid": "0000-0003-2879-5821" }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } } ] }, "title": "Enhanced sensitivity of the LIGO gravitational wave detector by using squeezed states of light", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2013 Macmillan Publishers Limited\n\nReceived: 23 April 2013. Accepted: 04 June 2013. Published online: 21 July 2013. \n\nThe authors acknowledge support from the United States National Science Foundation for the construction and operation of the LIGO Laboratory, and the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for supporting the construction and operation of the GEO600 detector. The authors also acknowledge support for the research, by these agencies and by the Australian Research Council, the International Science Linkages programme of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Econom\u00eda y Competitividad, the Conselleria d'Economia, Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the National Research Foundation of Korea, Industry Canada and the Province of Ontario through the Ministry of Economic Development and Innovation, the National Science and Engineering Research Council Canada, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation and the Alfred P. Sloan Foundation. \n\nAuthor Contributions: The activities of the LIGO Scientific Collaboration (LSC) include modelling astrophysical sources of gravitational waves, setting sensitivity requirements for observatories, designing, building and running observatories, carrying out research and development of new techniques to increase the sensitivity of these observatories, and performing searches for astrophysical signals contained in the data. S. Dwyer, S. Chua, L. Barsotti and D. Sigg were the leading scientists on this experiment, but a number of LSC members contributed directly to its success. M. Stefszky, A. Khalaidovski, M. Factourovich and C. Mow-Lowry assisted with the development of the squeezed vacuum source under the leadership of N. Mavalvala, D. McClelland and R. Schnabel. K. Kawabe supervised the integration of the squeezed vacuum source into the LIGO interferometer, with invaluable support from M. Landry and the LIGO Hanford Observatory staff. N. Smith-Lefebvre, M. Evans, R. Schofield and C. Vorvick kept the LIGO interferometer at its peak sensitivity and supported the integration of the squeezed vacuum source, with contributions from G. Meadors and D. Gustafson. The initial manuscript was written by L. Barsotti, N. Mavalvala, D. Sigg and D. McClelland. The LSC review of the manuscript was organized by S. Whitcomb. All authors approved the final version of the manuscript. \n\nThe authors declare no competing financial interests.\n\nSubmitted - 1310.0383v1.pdf
Supplemental Material - nphoton.2013.177-s1.pdf
", "abstract": "Nearly a century after Einstein first predicted the existence of gravitational waves, a global network of Earth-based gravitational wave observatories is seeking to directly detect this faint radiation using precision laser interferometry. Photon shot noise, due to the quantum nature of light, imposes a fundamental limit on the attometre-level sensitivity of the kilometre-scale Michelson interferometers deployed for this task. Here, we inject squeezed states to improve the performance of one of the detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) beyond the quantum noise limit, most notably in the frequency region down to 150 Hz, critically important for several astrophysical sources, with no deterioration of performance observed at any frequency. With the injection of squeezed states, this LIGO detector demonstrated the best broadband sensitivity to gravitational waves ever achieved, with important implications for observing the gravitational-wave Universe with unprecedented sensitivity.", "date": "2013-08", "date_type": "published", "publication": "Nature Photonics", "volume": "7", "number": "8", "publisher": "Nature Publishing Group", "pagerange": "613-619", "id_number": "CaltechAUTHORS:20140124-105938310", "issn": "1749-4885", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140124-105938310", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages programme of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Econom\u00eda y Competitividad (MINECO)" }, { "agency": "Conselleria d'Economia, Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "National Research Foundation of Korea" }, { "agency": "Industry Canada" }, { "agency": "Ontario Ministry of Economic Development and Innovation" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1038/NPHOTON.2013.177", "primary_object": { "basename": "1310.0383v1.pdf", "url": "https://authors.library.caltech.edu/records/rya2e-p1e42/files/1310.0383v1.pdf" }, "related_objects": [ { "basename": "nphoton.2013.177-s1.pdf", "url": "https://authors.library.caltech.edu/records/rya2e-p1e42/files/nphoton.2013.177-s1.pdf" } ], "resource_type": "article", "pub_year": "2013", "author_list": "Aasi, J.; Abadie, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/t59cm-z7k90", "eprint_id": 37335, "eprint_status": "archive", "datestamp": "2023-08-19 14:25:18", "lastmod": "2023-10-23 17:22:55", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Babak-S", "name": { "family": "Babak", "given": "S." } }, { "id": "Biswas-R", "name": { "family": "Biswas", "given": "R." }, "orcid": "0000-0002-5741-7195" }, { "id": "Brady-P-R", "name": { "family": "Brady", "given": "P. R." }, "orcid": "0000-0002-4611-9387" }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Cannon-K", "name": { "family": "Cannon", "given": "K." } }, { "id": "Capano-C-D", "name": { "family": "Capano", "given": "C. D." } }, { "id": "Clayton-J-H", "name": { "family": "Clayton", "given": "J. H." } }, { "id": "Cokelaer-T", "name": { "family": "Cokelaer", "given": "T." } }, { "id": "Creighton-J-D-E", "name": { "family": "Creighton", "given": "J. D. E." } }, { "id": "Dent-T", "name": { "family": "Dent", "given": "T." } }, { "id": "Dietz-A", "name": { "family": "Dietz", "given": "A." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fotopoulos-N", "name": { "family": "Fotopoulos", "given": "N." } }, { "id": "Gonz\u00e1lez-G", "name": { "family": "Gonz\u00e1lez", "given": "G." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Harry-I-W", "name": { "family": "Harry", "given": "I. W." } }, { "id": "Jones-G", "name": { "family": "Jones", "given": "G." } }, { "id": "Keppel-D", "name": { "family": "Keppel", "given": "D." } }, { "id": "McKechan-D-J-A", "name": { "family": "McKechan", "given": "D. J. A." } }, { "id": "Pekowsky-L", "name": { "family": "Pekowsky", "given": "L." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Robinson-C", "name": { "family": "Robinson", "given": "C." } }, { "id": "Rodriguez-A-C", "name": { "family": "Rodriguez", "given": "A. C." } }, { "id": "Sathyaprakash-B-S", "name": { "family": "Sathyaprakash", "given": "B. S." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vaulin-R", "name": { "family": "Vaulin", "given": "R." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Searching for gravitational waves from binary coalescence", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2013 American Physical Society.\n\nReceived 29 August 2012; published 22 January 2013.\n\nThe authors would like to thank their colleagues in the\nLIGO Scientific Collaboration and Virgo Collaboration,\nand particularly the other members of the Compact\nBinary Coalescence Search Group. The authors gratefully\nacknowledge the support of the United States National\nScience Foundation, the Science and Technology\nFacilities Council of the United Kingdom, the Royal\nSociety, the Max Planck Society, the National\nAeronautics and Space Administration, Industry Canada\nand the Province of Ontario through the Ministry of\nResearch and Innovation. LIGO was constructed by the\nCalifornia Institute of Technology and Massachusetts\nInstitute of Technology with funding from the National\nScience Foundation and operates under cooperative agreement\nPHY-0757058.\n\nPublished - PhysRevD.87.024033.pdf
Submitted - 1208.3491v1.pdf
", "abstract": "We describe the implementation of a search for gravitational waves from compact binary coalescences\nin LIGO and Virgo data. This all-sky, all-time, multidetector search for binary coalescence has been used\nto search data taken in recent LIGO and Virgo runs. The search is built around a matched filter analysis of\nthe data, augmented by numerous signal consistency tests designed to distinguish artifacts of non-\nGaussian detector noise from potential detections.We demonstrate the search performance using Gaussian\nnoise and data from the fifth LIGO science run and demonstrate that the signal consistency tests are\ncapable of mitigating the effect of non-Gaussian noise and providing a sensitivity comparable to that\nachieved in Gaussian noise.", "date": "2013-01-22", "date_type": "published", "publication": "Physical Review D", "volume": "87", "number": "2", "publisher": "American Physical Society", "pagerange": "Art. No. 024033", "id_number": "CaltechAUTHORS:20130306-090142836", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130306-090142836", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC) (UK)" }, { "agency": "Royal Society" }, { "agency": "Max Planck Society" }, { "agency": "NASA" }, { "agency": "Industry Canada" }, { "agency": "Ministry of Research and Innovation, Province of Ontario, Canada" }, { "agency": "NSF", "grant_number": "PHY-0757058" } ] }, "doi": "10.1103/PhysRevD.87.024033", "primary_object": { "basename": "1208.3491v1.pdf", "url": "https://authors.library.caltech.edu/records/t59cm-z7k90/files/1208.3491v1.pdf" }, "related_objects": [ { "basename": "PhysRevD.87.024033.pdf", "url": "https://authors.library.caltech.edu/records/t59cm-z7k90/files/PhysRevD.87.024033.pdf" } ], "resource_type": "article", "pub_year": "2013", "author_list": "Babak, S.; Biswas, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/xhs56-xwh79", "eprint_id": 35880, "eprint_status": "archive", "datestamp": "2023-08-22 07:11:24", "lastmod": "2023-10-20 21:53:12", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Nissanke-S", "name": { "family": "Nissanke", "given": "Samaya" } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" }, { "id": "Nelemans-G", "name": { "family": "Nelemans", "given": "Gijs" } }, { "id": "Prince-T-A", "name": { "family": "Prince", "given": "Thomas A." }, "orcid": "0000-0002-8850-3627" } ] }, "title": "Gravitational-wave Emission from Compact Galactic Binaries", "ispublished": "pub", "full_text_status": "public", "keywords": "binaries: close; Galaxy: general; gravitational waves; methods: data analysis; white dwarfs", "note": "\u00a9 2012 American Astronomical Society.\n\nReceived 2012 March 2; accepted 2012 July 12; published 2012 October 9.\n\nFor useful discussions and interactions,we are grateful to Lars Bildsten, Roseanne Di Stefano, Paul Groot, Mukremin Kilic, Shri Kulkarni, David Levitan, Avi Loeb, Sterl Phinney, Tony Piro, and Ken Shen. Part of this work was performed by TAP while at the Aspen Center for Physics, which is supported by NSF grant No. 1066293. G.N. is supported by NWO and FOM. M.V. is grateful for support from the LISA Mission Science Office. Part of this work was performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. Government sponsorship acknowledged. Copyright 2011.\n\nPublished - 0004-637X_758_2_131.pdf
", "abstract": "Compact Galactic binaries where at least one member is a white dwarf (WD) or neutron star constitute the majority of individually detectable sources for future low-frequency space-based gravitational-wave (GW) observatories; they also form an unresolved continuum, the dominant Galactic foreground at frequencies below a few mHz. Due to the paucity of electromagnetic observations, the majority of studies of Galactic-binary populations so far have been based on population-synthesis simulations. However, recent surveys have reported several new detections of WD binaries, providing new constraints for population estimates. In this article, we evaluate the impact of revised local densities of interacting WD binaries on future GW observations. Specifically, we consider five scenarios that explain these densities with different assumptions on the formation of interacting systems; we simulate corresponding populations of detached and interacting WD binaries; we estimate the number of individually detectable GW sources and the magnitude of the confusion-noise foreground, as observed by space-based detectors with 5 and 1 Mkm arms. We confirm earlier estimates of thousands of detached-binary detections, but project only a few ten to a few hundred detections of interacting systems. This reduction is partly due to our assessment of detection prospects, based on the iterative identification and subtraction of bright sources with respect to both instrument and confusion noise. We also confirm earlier estimates for the confusion-noise foreground, except in one scenario that explains smaller local densities of interacting systems with smaller numbers of progenitor detached systems.", "date": "2012-10-20", "date_type": "published", "publication": "Astrophysical Journal", "volume": "758", "number": "2", "publisher": "American Astronomical Society", "pagerange": "Art. No. 131", "id_number": "CaltechAUTHORS:20121207-132844562", "issn": "0004-637X", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20121207-132844562", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "PHY-1066293" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "LISA Mission Science Office" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "Space-Radiation-Laboratory" } ] }, "doi": "10.1088/0004-637X/758/2/131", "primary_object": { "basename": "0004-637X_758_2_131.pdf", "url": "https://authors.library.caltech.edu/records/xhs56-xwh79/files/0004-637X_758_2_131.pdf" }, "resource_type": "article", "pub_year": "2012", "author_list": "Nissanke, Samaya; Vallisneri, Michele; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/rvh81-87n78", "eprint_id": 33694, "eprint_status": "archive", "datestamp": "2023-08-22 06:23:24", "lastmod": "2023-10-18 20:34:50", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cannon-K", "name": { "family": "Cannon", "given": "K." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Dannenberg-R", "name": { "family": "Dannenberg", "given": "R." } }, { "id": "Daudert-B", "name": { "family": "Daudert", "given": "B." } }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Driggers-J-C", "name": { "family": "Driggers", "given": "J. C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Engel-R", "name": { "family": "Engel", "given": "R." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Harms-J", "name": { "family": "Harms", "given": "J." }, "orcid": "0000-0002-7332-9806" }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A-W", "name": { "family": "Heptonstall", "given": "A. W." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Korth-W-Z", "name": { "family": "Korth", "given": "W. Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Phelps-M", "name": { "family": "Phelps", "given": "M." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Singer-L", "name": { "family": "Singer", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A-E", "name": { "family": "Villar", "given": "A. E." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Boyle-M", "name": { "family": "Boyle", "given": "M." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Hong-T", "name": { "family": "Hong", "given": "T." } }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Implications for the Origin of GRB 051103 from LIGO Observations", "ispublished": "pub", "full_text_status": "public", "keywords": "gamma-ray burst: individual (GRB 051103); gravitational waves; stars: magnetars", "note": "\u00a9 2012 American Astronomical Society. Received 2012 February 6, accepted for publication 2012 May 26. Published 2012 July 19. The authors thank A. Rowlinson and N. Tanvir for bringing GRB 051103 to our attention. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the French Centre National de la Recherche Scientifique, the Spanish Ministerio de Educaci\u03ccn y Ciencia, the Conselleria d'Economia, Hisenda i Innovaci\u03cc of the Govern de les Illes Balears, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory document number LIGO-P10000097-v12.\n\nPublished - 0004-637X_755_1_2.pdf
", "abstract": "We present the results of a LIGO search for gravitational waves (GWs) associated with GRB 051103, a short-duration hard-spectrum gamma-ray burst (GRB) whose electromagnetically determined sky position is coincident with the spiral galaxy M81, which is 3.6 Mpc from Earth. Possible progenitors for short-hard GRBs include compact object mergers and soft gamma repeater (SGR) giant flares. A merger progenitor would produce a characteristic GW signal that should be detectable at a distance of M81, while GW emission from an SGR is not expected to be detectable at that distance. We found no evidence of a GW signal associated with GRB 051103. Assuming weakly beamed \u03b3-ray emission with a jet semi-angle of 30\u00b0, we exclude a binary neutron star merger in M81 as the progenitor with a confidence of 98%. Neutron star-black hole mergers are excluded with >99% confidence. If the event occurred in M81, then our findings support the hypothesis that GRB 051103 was due to an SGR giant flare, making it one of the most distant extragalactic magnetars observed to date.", "date": "2012-08-10", "date_type": "published", "publication": "Astrophysical Journal", "volume": "755", "number": "1", "publisher": "American Astronomical Society", "pagerange": "Art. No. 2", "id_number": "CaltechAUTHORS:20120829-154041074", "issn": "0004-637X", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20120829-154041074", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P10000097-v12", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1088/0004-637X/755/1/2", "primary_object": { "basename": "0004-637X_755_1_2.pdf", "url": "https://authors.library.caltech.edu/records/rvh81-87n78/files/0004-637X_755_1_2.pdf" }, "resource_type": "article", "pub_year": "2012", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/sgqsx-jfh66", "eprint_id": 37319, "eprint_status": "archive", "datestamp": "2023-08-19 11:26:47", "lastmod": "2023-10-23 17:21:59", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" }, { "id": "Galley-C-R", "name": { "family": "Galley", "given": "Chad R." } } ] }, "title": "Non-sky-averaged sensitivity curves for space-based gravitational-wave observatories", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2012 IOP Publishing Ltd. \n\nReceived 23 January 2012, in final form 20 March 2012. Published 1 June 2012. \n\nMV is grateful to J Armstrong, F Estabrook and M Tinto for teaching him about TDI and sensitivity calculations. This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. MV was supported by the LISA Mission Science Office and by the JPL RTD program. CG was supported by an appointment to the NASA Postdoctoral Program at the JPL administered by Oak Ridge Associated Universities through a contract with NASA. Copyright 2012 California Institute of Technology.\n\nPublished - Vallisneri_2012_Class._Quantum_Grav._29_124015.pdf
Submitted - 1201.3684.pdf
Supplemental Material - SensitivityDistribution-120410.nb
", "abstract": "The signal-to-noise ratio (SNR) is used in gravitational-wave observations as the basic figure of merit for detection confidence and, together with the Fisher matrix, for the amount of physical information that can be extracted from a detected signal. SNRs are usually computed from a sensitivity curve, which describes the gravitational-wave amplitude needed by a monochromatic source of given frequency to achieve a threshold SNR. Although the term 'sensitivity' is used loosely to refer to the detector's noise spectral density, the two quantities are not the same: the sensitivity includes also the frequency- and orientation-dependent response of the detector to gravitational waves and takes into account the duration of observation. For interferometric space-based detectors similar to LISA, which are sensitive to long-lived signals and have constantly changing position and orientation, exact SNRs need to be computed on a source-by-source basis. For convenience, most authors prefer to work with sky-averaged sensitivities, accepting inaccurate SNRs for individual sources and giving up control over the statistical distribution of SNRs for source populations. In this paper, we describe a straightforward end-to-end recipe to compute the non-sky-averaged sensitivity of interferometric space-based detectors of any geometry. This recipe includes the effects of spacecraft motion and of seasonal variations in the partially subtracted confusion foreground from Galactic binaries, and it can be used to generate a sampling distribution of sensitivities for a given source population. In effect, we derive error bars for the sky-averaged sensitivity curve, which provide a stringent statistical interpretation for previously unqualified statements about sky-averaged SNRs. As a worked-out example, we consider isotropic and Galactic-disk populations of monochromatic sources, as observed with the 'classic LISA' configuration. We confirm that the (standard) inverse-rms average sensitivity for the isotropic population remains the same whether or not the LISA orbits are included in the computation. However, detector motion tightens the distribution of sensitivities, so for 50% of sources the sensitivity is within 30% of its average. For the Galactic-disk population, the average and the distribution of the sensitivity for a moving detector turn out to be similar to the isotropic case.", "date": "2012-06-21", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "29", "number": "12", "publisher": "IOP", "pagerange": "Art. No. 124015", "id_number": "CaltechAUTHORS:20130305-143752417", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130305-143752417", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NASA/JPL/Caltech" }, { "agency": "JPL Research and Technology Development Fund" }, { "agency": "NASA Postdoctoral Program" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/29/12/124015", "primary_object": { "basename": "1201.3684.pdf", "url": "https://authors.library.caltech.edu/records/sgqsx-jfh66/files/1201.3684.pdf" }, "related_objects": [ { "basename": "SensitivityDistribution-120410.nb", "url": "https://authors.library.caltech.edu/records/sgqsx-jfh66/files/SensitivityDistribution-120410.nb" }, { "basename": "Vallisneri_2012_Class._Quantum_Grav._29_124015.pdf", "url": "https://authors.library.caltech.edu/records/sgqsx-jfh66/files/Vallisneri_2012_Class._Quantum_Grav._29_124015.pdf" } ], "resource_type": "article", "pub_year": "2012", "author_list": "Vallisneri, Michele and Galley, Chad R." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/qcvxc-t5w31", "eprint_id": 31545, "eprint_status": "archive", "datestamp": "2023-08-19 10:40:41", "lastmod": "2023-10-17 18:39:35", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Corsi-A", "name": { "family": "Corsi", "given": "A." }, "orcid": "0000-0001-8104-3536" }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. 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R." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Santamaria-L", "name": { "family": "Santamaria", "given": "L." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Singer-L", "name": { "family": "Singer", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A-E", "name": { "family": "Villar", "given": "A. E." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Harms-J", "name": { "family": "Harms", "given": "J." }, "orcid": "0000-0002-7332-9806" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Marandi-A", "name": { "family": "Marandi", "given": "A." }, "orcid": "0000-0002-0470-0050" } ] }, "title": "Search for gravitational waves from low mass compact binary coalescence in LIGO's sixth science run and Virgo's science runs 2 and 3", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2012 American Physical Society. \n\nReceived 16 December 2011; published 19 April 2012. \n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory, the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector, and the Italian\nIstituto Nazionale di Fisica Nucleare and the French\nCentre National de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors\nalso gratefully acknowledge the support of the research by\nthese agencies and by the Australian Research Council,\nthe International Science Linkages program of the\nCommonwealth of Australia, the Council of Scientific\nand Industrial Research of India, the Istituto Nazionale di\nFisica Nucleare of Italy, the Spanish Ministerio de\nEducaci\u03ccn y Ciencia, the Conselleria d'Economia\nHisenda i Innovaci\u03cc of the Govern de les Illes Balears,\nthe Foundation for Fundamental Research on Matter supported\nby the Netherlands Organisation for Scientific\nResearch, the Polish Ministry of Science and Higher\nEducation, the FOCUS Programme of Foundation for\nPolish Science, the Royal Society, the Scottish Funding\nCouncil, the Scottish Universities Physics Alliance, the\nNational Aeronautics and Space Administration, the\nCarnegie Trust, the Leverhulme Trust, the David and\nLucile Packard Foundation, the Research Corporation,\nand the Alfred P. Sloan Foundation.\n\nPublished - Abadie2012p18158Phys_Rev_D.pdf
Submitted - 1111.7314.pdf
", "abstract": "We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo observations between July 7, 2009, and October 20, 2010. We searched for signals from binaries with total mass between 2 and 25M_\u2299; this includes binary neutron stars, binary black holes, and binaries consisting of a black hole and neutron star. The detectors were sensitive to systems up to 40 Mpc distant for binary neutron stars, and further for higher mass systems. No gravitational-wave signals were detected. We report upper limits on the rate of compact binary coalescence as a function of total mass, including the results from previous LIGO and Virgo observations. The cumulative 90% confidence rate upper limits of the binary coalescence of binary neutron star, neutron star-black hole, and binary black hole systems are 1.3\u00d710^(-4), 3.1\u00d710^(-5), and 6.4\u00d710^(-6)\u2009\u2009Mpc^(-3)\u2009yr^(-1), respectively. These upper limits are up to a factor 1.4 lower than previously derived limits. We also report on results from a blind injection challenge.", "date": "2012-04-19", "date_type": "published", "publication": "Physical Review D", "volume": "85", "number": "8", "publisher": "American Physical Society", "pagerange": "Art. No. 082002", "id_number": "CaltechAUTHORS:20120518-143548930", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20120518-143548930", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.85.082002", "primary_object": { "basename": "1111.7314.pdf", "url": "https://authors.library.caltech.edu/records/qcvxc-t5w31/files/1111.7314.pdf" }, "related_objects": [ { "basename": "Abadie2012p18158Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/qcvxc-t5w31/files/Abadie2012p18158Phys_Rev_D.pdf" } ], "resource_type": "article", "pub_year": "2012", "author_list": "Abadie, J.; Abbott, B. 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S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A-E", "name": { "family": "Villar", "given": "A. E." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Hong-T", "name": { "family": "Hong", "given": "T." } }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Harms-J", "name": { "family": "Harms", "given": "J." }, "orcid": "0000-0002-7332-9806" }, { "id": "Ofek-E-O", "name": { "family": "Ofek", "given": "E. O." }, "orcid": "0000-0002-6786-8774" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Implementation and testing of the first prompt search\n for gravitational wave transients with electromagnetic counterparts", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; methods: observational", "note": "\u00a9 2012 ESO. Received: 6 October 2011. Accepted: 22 December 2011. Published online:\t29 March 2012. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge\nthe support of gravitational wave research by these agencies and by the Australian Research Council, the International Science Linkages program of the Commonwealth of Australia, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u00f3n y Ciencia, the Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by The Netherlands Organisation for Scientific Research, the\nPolish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space\nAdministration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. The authors acknowledge support for TAROT from the French Minist\u00e8re des Affaires \u00c9trang\u00e8res and Minist\u00e8re de l'Enseignement Sup\u00e9rieur et\nde la Recherche. The observations by ROTSE-III were supported by NASA grant NNX08AV63G and NSF grant PHY-0801007. The work with Swift was partially supported through a NASA grant/cooperative agreement number NNX09AL61G to the Massachusetts Institute of Technology. The contribution from the \"Pi of the Sky\" group was financed by the Polish Ministry of Science in 2008-2011 as a research project. We thank Joshua S. Bloom for useful discussions on the rates of PTF transients and their classification. This document has been assigned\nLIGO Laboratory document number LIGO-P1000061-v19.\n\nPublished - Abadie2012p18477Astron_Astrophys.pdf
", "abstract": "Aims. A transient astrophysical event observed in both gravitational wave (GW) and electromagnetic (EM) channels would yield rich scientific rewards. A first program initiating EM follow-ups to possible transient GW events has been developed and exercised by the LIGO and Virgo community in association with several partners. In this paper, we describe and evaluate the methods used to promptly identify and localize GW event candidates and to request images of targeted sky locations.\n\nMethods. During two observing periods (Dec. 17, 2009 to Jan. 8, 2010 and Sep. 2 to Oct. 20, 2010), a low-latency analysis pipeline was used to identify GW event candidates and to reconstruct maps of possible sky locations. A catalog of nearby galaxies and Milky Way globular clusters was used to select the most promising sky positions to be imaged, and this directional information was delivered to EM observatories with time lags of about thirty minutes. A Monte Carlo simulation has been used to evaluate the low-latency GW pipeline's ability to reconstruct source positions correctly.\n\nResults. For signals near the detection threshold, our low-latency algorithms often localized simulated GW burst signals to tens of square degrees, while neutron star/neutron star inspirals and neutron star/black hole inspirals were localized to a few hundred square degrees. Localization precision improves for moderately stronger signals. The correct sky location of signals well above threshold and originating from nearby galaxies may be observed with ~50% or better probability with a few pointings of wide-field telescopes.", "date": "2012-03", "date_type": "published", "publication": "Astronomy and Astrophysics", "volume": "539", "publisher": "EDP Sciences", "pagerange": "Art. No. A124", "id_number": "CaltechAUTHORS:20120619-081035905", "issn": "0004-6361", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20120619-081035905", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Minist\u00e8re des Affaires Etrang\u00e8res" }, { "agency": "Minist\u00e8re de'l Enseignement Sup\u00e9rieur et de la Recherche" }, { "agency": "NASA", "grant_number": "NNX08AV63G" }, { "agency": "NSF", "grant_number": "PHY-0801007" }, { "agency": "NASA", "grant_number": "NNX09AL61G" }, { "agency": "Ministry of Science (Poland)" }, { "agency": "Max-Planck-Society" } ] }, "other_numbering_system": { "items": [ { "id": "P1000061-v19", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "Palomar-Transient-Factory" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1051/0004-6361/201118219", "primary_object": { "basename": "Abadie2012p18477Astron_Astrophys.pdf", "url": "https://authors.library.caltech.edu/records/ax7wj-78a15/files/Abadie2012p18477Astron_Astrophys.pdf" }, "resource_type": "article", "pub_year": "2012", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/bs3pt-rjn26", "eprint_id": 29158, "eprint_status": "archive", "datestamp": "2023-08-19 09:35:45", "lastmod": "2023-10-24 18:24:25", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Corsi-A", "name": { "family": "Corsi", "given": "A." }, "orcid": "0000-0001-8104-3536" }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. 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N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Phelps-M", "name": { "family": "Phelps", "given": "M." } }, { "id": "Price-L-R", "name": { "family": "Price", "given": "L. R." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Santamar\u00eda-L", "name": { "family": "Santamar\u00eda", "given": "L." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Singer-L", "name": { "family": "Singer", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A-E", "name": { "family": "Villar", "given": "A. E." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "All-sky search for periodic gravitational waves in the full S5 LIGO data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2012 American Physical Society.\n\nReceived 24 October 2011; published 5 January 2012.\n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the\nconstruction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector, and the Italian\nIstituto Nazionale di Fisica Nucleare and the French\nCentre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the International Science Linkages program of the\nCommonwealth of Australia, the Council of Scientific\nand Industrial Research of India, the Istituto Nazionale di\nFisica Nucleare of Italy, the Spanish Ministerio de\nEducaci\u03ccn y Ciencia, the Conselleria d'Economia\nHisenda i Innovaci\u03cc of the Govern de les Illes Balears,\nthe Foundation for Fundamental Research on Matter supported\nby the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory Document No. LIGO-P1100029-v36.\n\nPublished - Abadie2012p17001Phys_Rev_D.pdf
Submitted - 1110.0208v1.pdf
Supplemental Material - README.TXT
Supplemental Material - README.data
Supplemental Material - upper_limits.csv
", "abstract": "We report on an all-sky search for periodic gravitational waves in the frequency band 50\u2013800 Hz and with the frequency time derivative in the range of 0 through -6\u00d710^(-9)\u2009\u2009Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our Galaxy. After recent improvements in the search program that yielded a 10\u00d7 increase in computational efficiency, we have searched in two years of data collected during LIGO's fifth science run and have obtained the most sensitive all-sky upper limits on gravitational-wave strain to date. Near 150 Hz our upper limit on worst-case linearly polarized strain amplitude h_0 is 1\u00d710^(-24), while at the high end of our frequency range we achieve a worst-case upper limit of 3.8\u00d710^(-24) for all polarizations and sky locations. These results constitute a factor of 2 improvement upon previously published data. A new detection pipeline utilizing a loosely coherent algorithm was able to follow up weaker outliers, increasing the volume of space where signals can be detected by a factor of 10, but has not revealed any gravitational-wave signals. The pipeline has been tested for robustness with respect to deviations from the model of an isolated neutron star, such as caused by a low-mass or long-period binary companion.", "date": "2012-01-15", "date_type": "published", "publication": "Physical Review D", "volume": "85", "number": "2", "publisher": "American Physical Society", "pagerange": "Art. No. 022001", "id_number": "CaltechAUTHORS:20120206-151908677", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20120206-151908677", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "International Science Linkages program of the Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P1100029-v36", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.85.022001", "primary_object": { "basename": "1110.0208v1.pdf", "url": "https://authors.library.caltech.edu/records/bs3pt-rjn26/files/1110.0208v1.pdf" }, "related_objects": [ { "basename": "Abadie2012p17001Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/bs3pt-rjn26/files/Abadie2012p17001Phys_Rev_D.pdf" }, { "basename": "README.TXT", "url": "https://authors.library.caltech.edu/records/bs3pt-rjn26/files/README.TXT" }, { "basename": "README.data", "url": "https://authors.library.caltech.edu/records/bs3pt-rjn26/files/README.data" }, { "basename": "upper_limits.csv", "url": "https://authors.library.caltech.edu/records/bs3pt-rjn26/files/upper_limits.csv" } ], "resource_type": "article", "pub_year": "2012", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/26hhm-0np13", "eprint_id": 29019, "eprint_status": "archive", "datestamp": "2023-08-19 09:01:19", "lastmod": "2023-10-24 18:18:48", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Harms-J", "name": { "family": "Harms", "given": "J." }, "orcid": "0000-0002-7332-9806" }, { "id": "Boyle-M", "name": { "family": "Boyle", "given": "M." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. 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S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Turner-L", "name": { "family": "Turner", "given": "L." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A-E", "name": { "family": "Villar", "given": "A. E." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Directional Limits on Persistent Gravitational Waves Using LIGO S5 Science Data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2011 American Physical Society. Received 9 October 2011; published 29 December 2011. The authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory, the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector, and the Italian\nIstituto Nazionale di Fisica Nucleare and the French\nCentre National de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors\nalso gratefully acknowledge the support of the research by\nthese agencies and by the Australian Research Council, the\nInternational Science Linkages program of the\nCommonwealth of Australia, the Council of Scientific\nand Industrial Research of India, the Istituto Nazionale di\nFisica Nucleare of Italy, the Spanish Ministerio de\nEducacio\u00b4n y Ciencia, the Conselleria d'Economia\nHisenda i Innovacio\u00b4 of the Govern de les Illes Balears,\nthe Foundation for Fundamental Research on Matter supported\nby the Netherlands Organisation for Scientific\nResearch, the Polish Ministry of Science and Higher\nEducation, the FOCUS Programme of Foundation for\nPolish Science, the Royal Society, the Scottish Funding\nCouncil, the Scottish Universities Physics Alliance, The\nNational Aeronautics and Space Administration, the\nCarnegie Trust, the Leverhulme Trust, the David and\nLucile Packard Foundation, the Research Corporation,\nand the Alfred P. Sloan Foundation.\n\nPublished - Abadie2011p16900Phys_Rev_Lett.pdf
", "abstract": "The gravitational-wave (GW) sky may include nearby pointlike sources as well as stochastic backgrounds. We perform two directional searches for persistent GWs using data from the LIGO S5 science run: one optimized for pointlike sources and one for arbitrary extended sources. Finding no evidence to support the detection of GWs, we present 90% confidence level (C.L.) upper-limit maps of GW strain power with typical values between 2-20\u00d710^(-50)\u2009\u2009strain^2\u2009Hz^(-1) and 5-35\u00d710^(-49)\u2009\u2009strain^2\u2009Hz^(-1)\u2009sr^(-1) for pointlike and extended sources, respectively. The latter result is the first of its kind. We also set 90% C.L. limits on the narrow-band root-mean-square GW strain from interesting targets including Sco X-1, SN 1987A and the Galactic center as low as \u22487\u00d710^(-25) in the most sensitive frequency range near 160 Hz.", "date": "2011-12-29", "date_type": "published", "publication": "Physical Review Letters", "volume": "107", "number": "27", "publisher": "American Physical Society", "pagerange": "Art. No. 271102", "id_number": "CaltechAUTHORS:20120130-113016680", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20120130-113016680", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Commonwealth of Australia" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevLett.107.271102", "primary_object": { "basename": "Abadie2011p16900Phys_Rev_Lett.pdf", "url": "https://authors.library.caltech.edu/records/26hhm-0np13/files/Abadie2011p16900Phys_Rev_Lett.pdf" }, "resource_type": "article", "pub_year": "2011", "author_list": "Abadie, J.; Drever, R. W. 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A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Hong-T-M", "name": { "family": "Hong", "given": "T." } }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } } ] }, "title": "A gravitational wave observatory operating beyond the quantum shot-noise limit", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2011 Macmillan Publishers Limited.\n\nReceived 11 May 2011; Accepted 03 August 2011; Published\n11 September 2011.\n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Science and Technology Facilities Council of the United Kingdom, the Max Planck Society, the Deutsche Forschungsgemeinschaft, the cluster of excellence QUEST (Centre for Quantum Engineering and Space-Time Research), the BMBF, the Volkswagen Foundation, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO\u2009600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the International Max Planck Research School (IMPRS), the SFB\u2009TR7, the FP7 project Q-ESSENCE, the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u00f3n y Ciencia, the Conselleria d'Economia, Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the A. P. Sloan Foundation.\n\nContributions:\nA list of authors and their affiliations appear in the Supplementary Information The activities of the LIGO Scientific Collaboration (LSC) cover modelling astrophysical sources of gravitational waves, setting sensitivity requirements of observatories, designing, building and running observatories and researching new techniques to increase the sensitivity of these observatories, and performing searches for astrophysical signals contained in the data. The principal investigators of the advancement reported here are H.G. and R.S., being responsible for GEO\u2009600 and for the squeezed-light laser during the past 3 years, in which this experiment was prepared and conducted, respectively. In this period a great number of the LSC members contributed directly to the success of this project. H.V. and H.G. supervised the integration of the squeezed-light laser into GEO\u2009600. Together with A.K., they took and analysed the data shown. The initial manuscript was written by a team involving those mentioned above together with R.S. The manuscript went into a two-stage LSC-wide review process, which was organized and led by R.F., T.R.C., M.H., and D. Sigg. All authors approved the final version of the manuscript. \n\nThe author declare no competing financial interests.\n\nSubmitted - 1109.2295.pdf
Supplemental Material - nphys2083-s1.pdf
", "abstract": "Around the globe several observatories are seeking the first direct detection of gravitational waves (GWs). These waves are predicted by Einstein's general theory of relativity and are generated, for example, by black-hole binary systems. Present GW detectors are Michelson-type kilometre-scale laser interferometers measuring the distance changes between mirrors suspended in vacuum. The sensitivity of these detectors at frequencies above several hundred hertz is limited by the vacuum (zero-point) fluctuations of the electromagnetic field. A quantum technology\u2014the injection of squeezed light\u2014offers a solution to this problem. Here we demonstrate the squeezed-light enhancement of GEO\u2009600, which will be the GW observatory operated by the LIGO Scientific Collaboration in its search for GWs for the next 3\u20134 years. GEO\u2009600 now operates with its best ever sensitivity, which proves the usefulness of quantum entanglement and the qualification of squeezed light as a key technology for future GW astronomy.", "date": "2011-12", "date_type": "published", "publication": "Nature Physics", "volume": "7", "number": "12", "publisher": "Nature Publishing Group", "pagerange": "962-965", "id_number": "CaltechAUTHORS:20180611-155020083", "issn": "1745-2473", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180611-155020083", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "Centre for Quantum Engineering and Space-Time Research" }, { "agency": "Bundesministerium f\u00fcr Bildung und Forschung (BMBF)" }, { "agency": "Volkswagen Foundation" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "International Max Planck Research School (IMPRS) for Astronomy and Astrophysics" }, { "agency": "Deutsche Forschungsgemeinschaft (DFG)", "grant_number": "SFB TR7" }, { "agency": "European Research Council (ERC)", "grant_number": "Q-ESSENCE" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia, Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1038/NPHYS2083", "primary_object": { "basename": "1109.2295.pdf", "url": "https://authors.library.caltech.edu/records/4n1gd-j2h68/files/1109.2295.pdf" }, "related_objects": [ { "basename": "nphys2083-s1.pdf", "url": "https://authors.library.caltech.edu/records/4n1gd-j2h68/files/nphys2083-s1.pdf" } ], "resource_type": "article", "pub_year": "2011", "author_list": "Abadie, J.; Marandi, A.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/saafw-kqb87", "eprint_id": 25270, "eprint_status": "archive", "datestamp": "2023-08-22 03:27:24", "lastmod": "2023-10-24 15:45:04", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Parameswaran-A", "name": { "family": "Parameswaran", "given": "A." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Phelps-M", "name": { "family": "Phelps", "given": "M." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Singer-L", "name": { "family": "Singer", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Turner-L", "name": { "family": "Turner", "given": "L." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A-E", "name": { "family": "Villar", "given": "A. E." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Marandi-A", "name": { "family": "Marandi", "given": "A." }, "orcid": "0000-0002-0470-0050" } ] }, "title": "Beating the Spin-down Limit on Gravitational Wave Emission from the Vela Pulsar", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; pulsars: individual (PSR J0835\u20134510); stars: neutron", "note": "\u00a9 2011 The American Astronomical Society. \n\nReceived 2011 May 3; accepted 2011 June 11; published 2011 August 8. \n\nThe authors gratefully acknowledge the support of the United\nStates National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology\nFacilities Council of the United Kingdom, the Max-Planck-\nSociety, the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u03ccn y Ciencia,\nthe Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern\nde les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities\nPhysics Alliance, The National Aeronautics and Space\nAdministration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - Abadie2011p15732Astrophys_J.pdf
Submitted - 1104.2712.pdf
", "abstract": "We present direct upper limits on continuous gravitational wave emission from the Vela pulsar using data from the Virgo detector's second science run. These upper limits have been obtained using three independent methods that assume the gravitational wave emission follows the radio timing. Two of the methods produce frequentist upper limits for an assumed known orientation of the star's spin axis and value of the wave polarization angle of, respectively, 1.9 \u00d7 10^(\u201324) and 2.2 \u00d7 10^(\u201324), with 95% confidence. The third method, under the same hypothesis, produces a Bayesian upper limit of 2.1 \u00d7 10^(\u201324), with 95% degree of belief. These limits are below the indirect spin-down limit of 3.3 \u00d7 10^(\u201324) for the Vela pulsar, defined by the energy loss rate inferred from observed decrease in Vela's spin frequency, and correspond to a limit on the star ellipticity of ~10^(\u20133). Slightly less stringent results, but still well below the spin-down limit, are obtained assuming the star's spin axis inclination and the wave polarization angles are unknown.", "date": "2011-08-20", "date_type": "published", "publication": "Astrophysical Journal", "volume": "737", "number": "2", "publisher": "American Astronomical Society", "pagerange": "Art. No. 93", "id_number": "CaltechAUTHORS:20110909-103003031", "issn": "0004-637X", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110909-103003031", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1088/0004-637X/737/2/93", "primary_object": { "basename": "1104.2712.pdf", "url": "https://authors.library.caltech.edu/records/saafw-kqb87/files/1104.2712.pdf" }, "related_objects": [ { "basename": "Abadie2011p15732Astrophys_J.pdf", "url": "https://authors.library.caltech.edu/records/saafw-kqb87/files/Abadie2011p15732Astrophys_J.pdf" } ], "resource_type": "article", "pub_year": "2011", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/fzea0-zyx12", "eprint_id": 25132, "eprint_status": "archive", "datestamp": "2023-08-22 02:57:35", "lastmod": "2023-10-24 15:38:57", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Arai-Koji", "name": { "family": "Arai", "given": "K." }, "orcid": "0000-0001-8916-8915" }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. C." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boyle-M", "name": { "family": "Boyle", "given": "M." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cannon-K", "name": { "family": "Cannon", "given": "K." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Dannenberg-R", "name": { "family": "Dannenberg", "given": "R." } }, { "id": "Daubert-B", "name": { "family": "Daubert", "given": "B." } }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Driggers-J-C", "name": { "family": "Driggers", "given": "J. 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G." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Korth-W-Z", "name": { "family": "Korth", "given": "W. Z." }, "orcid": "0000-0003-3527-1348" }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Ott-C-D", "name": { "family": "Ott", "given": "C. D." }, "orcid": "0000-0003-4993-2055" }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Parameswaran-A", "name": { "family": "Parameswaran", "given": "A." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Phelps-M", "name": { "family": "Phelps", "given": "M." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Singer-L", "name": { "family": "Singer", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Somiya-K", "name": { "family": "Somiya", "given": "K." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A-E", "name": { "family": "Villar", "given": "A. E." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yang-H", "name": { "family": "Yang", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Marandi-A", "name": { "family": "Marandi", "given": "A." }, "orcid": "0000-0002-0470-0050" } ] }, "title": "Search for Gravitational Wave Bursts from Six Magnetars", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; stars: magnetars", "note": "\u00a9 2011 The American Astronomical Society. Received 2010 December 6; accepted 2011 April 5; published 2011 June 1. The authors gratefully acknowledge the support of the United\nStates National Science Foundation for the construction and operation\nof the LIGO Laboratory, the Science and Technology\nFacilities Council of the United Kingdom, the Max-Planck-\nSociety, and the State of Niedersachsen/Germany for support\nof the construction and operation of the GEO600 detector, and\nthe Italian Istituto Nazionale di Fisica Nucleare and the French\nCentre National de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the Council\nof Scientific and Industrial Research of India, the Istituto\nNazionale di Fisica Nucleare of Italy, the Spanish Ministerio\nde Educaci\u00f3n y Ciencia, the Conselleria d'Economia Hisenda\ni Innovaci\u00f3 of the Govern de les Illes Balears, the Foundation\nfor Fundamental Research on Matter supported by the\nNetherlands Organisation for Scientific Research, the Polish\nMinistry of Science and Higher Education, the FOCUS Programme\nof Foundation for Polish Science, the Royal Society,\nthe Scottish Funding Council, the Scottish Universities Physics\nAlliance, The National Aeronautics and Space Administration,\nthe Carnegie Trust, the Leverhulme Trust, the David and Lucile\nPackard Foundation, the Research Corporation, and the Alfred\nP. Sloan Foundation. The Konus-Wind experiment is supported\nby a Russian Space Agency contract and RFBR grant 09-02-\n00166a. A.J.v.d.H. is supported by the NASA Postdoctoral\nProgram. K.H. acknowledges IPN support under the following\ngrants: JPL Y503559 (Odyssey); NASA NNG06GH00G,\nNASA NNX07AM42G, and NASA NNX08AC89G (INTEGRAL);\nNASA NNG06GI896, NASA NNX07AJ65G, and\nNASA NNX08AN23G (Swift); NASA NNX07AR71G (MESSENGER);\nNASA NNX06AI36G, NASA NNX08AB84G,\nNASA NNX08AZ85G (Suzaku); and NASA NNX09AU03G\n(Fermi). Y.K. acknowledges EU FP6 Project MTKD-CT-\n2006-042722. C.K. acknowledges support from NASA grant\nNNH07ZDA001-GLAST. This Letter is LIGO-P0900192.\n\nPublished - Abadie2011p15627Astrophys_J_Lett.pdf
Submitted - 1011.4079.pdf
", "abstract": "Soft gamma repeaters (SGRs) and anomalous X-ray pulsars (AXPs) are thought to be magnetars: neutron stars powered by extreme magnetic fields. These rare objects are characterized by repeated and sometimes spectacular gamma-ray bursts. The burst mechanism might involve crustal fractures and excitation of non-radial modes which would emit gravitational waves (GWs). We present the results of a search for GW bursts from six galactic magnetars that is sensitive to neutron star f-modes, thought to be the most efficient GW emitting oscillatory modes in compact stars. One of them, SGR 0501+4516, is likely ~1 kpc from Earth, an order of magnitude closer than magnetars targeted in previous GW searches. A second, AXP 1E 1547.0\u20135408, gave a burst with an estimated isotropic energy >10^(44) erg which is comparable to the giant flares. We find no evidence of GWs associated with a sample of 1279 electromagnetic triggers from six magnetars occurring between 2006 November and 2009 June, in GW data from the LIGO, Virgo, and GEO600 detectors. Our lowest model-dependent GW emission energy upper limits for band- and time-limited white noise bursts in the detector sensitive band, and for f-mode ringdowns (at 1090 Hz), are 3.0 \u00d7 10^(44) d^2_1 erg and 1.4 \u00d7 10^(47) d^2_1 erg, respectively, where d_1 = ^(d0501)_(1kpc) and d_ (0501) is the distance to SGR 0501+4516. These limits on GW emission from f-modes are an order of magnitude lower than any previous, and approach the range of electromagnetic energies seen in SGR giant flares for the first time.", "date": "2011-06-20", "date_type": "published", "publication": "Astrophysical Journal Letters", "volume": "734", "number": "2", "publisher": "American Astronomical Society", "pagerange": "Art. No. L35", "id_number": "CaltechAUTHORS:20110826-142324216", "issn": "2041-8205", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110826-142324216", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Russian Space Agency", "grant_number": "09-02-00166a" }, { "agency": "NASA Postdoctoral Program" }, { "agency": "JPL", "grant_number": "Y503559" }, { "agency": "NASA", "grant_number": "NNG06GH00G" }, { "agency": "NASA", "grant_number": "NNX07AM42G" }, { "agency": "NASA", "grant_number": "NNX08AC89G" }, { "agency": "NASA", "grant_number": "NNG06GI896" }, { "agency": "NASA", "grant_number": "NNX07AJ65G" }, { "agency": "NASA", "grant_number": "NNX08AN23G" }, { "agency": "NASA", "grant_number": "NNX07AR71G" }, { "agency": "NASA", "grant_number": "NNX06AI36G" }, { "agency": "NASA", "grant_number": "NNX08AB84G" }, { "agency": "NASA", "grant_number": "NNX08AZ85G" }, { "agency": "NASA", "grant_number": "NNX09AU03G" }, { "agency": "European Union (EU)", "grant_number": "MTKD-CT-2006-042722" }, { "agency": "NASA", "grant_number": "NNH07ZDA001-GLAST" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Russian Foundation for Basic Research" } ] }, "other_numbering_system": { "items": [ { "id": "P0900192", "name": "LIGO" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1088/2041-8205/734/2/L35", "primary_object": { "basename": "Abadie2011p15627Astrophys_J_Lett.pdf", "url": "https://authors.library.caltech.edu/records/fzea0-zyx12/files/Abadie2011p15627Astrophys_J_Lett.pdf" }, "related_objects": [ { "basename": "1011.4079.pdf", "url": "https://authors.library.caltech.edu/records/fzea0-zyx12/files/1011.4079.pdf" } ], "resource_type": "article", "pub_year": "2011", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/32x62-3re57", "eprint_id": 24052, "eprint_status": "archive", "datestamp": "2023-08-19 07:06:02", "lastmod": "2023-10-23 20:16:34", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M-C", "name": { "family": "Araya", "given": "M. 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C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Engel-R", "name": { "family": "Engel", "given": "R." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Harms-J", "name": { "family": "Harms", "given": "J." }, "orcid": "0000-0002-7332-9806" }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A-W", "name": { "family": "Heptonstall", "given": "A. W." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mak-C", "name": { "family": "Mak", "given": "C." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Mitra-S", "name": { "family": "Mitra", "given": "S." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Turner-L", "name": { "family": "Turner", "given": "L." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A-E", "name": { "family": "Villar", "given": "A. E." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for gravitational waves from binary black hole inspiral, merger, and ringdown", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2011 American Physical Society. Received 8 March 2011; published 6 June 2011. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French\nCentre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u03ccn y Ciencia, the Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears, the Foundation for Fundamental Research\non Matter supported by the Netherlands Organisation for\nScientific Research, the Polish Ministry of Science and\nHigher Education, the FOCUS Programme of Foundation\nfor Polish Science, the Royal Society, the Scottish Funding\nCouncil, the Scottish Universities Physics Alliance, The\nNational Aeronautics and Space Administration, the\nCarnegie Trust, the Leverhulme Trust, the David and\nLucile Packard Foundation, the Research Corporation,\nand the Alfred P. Sloan Foundation.\n\nPublished - Abadie2011p14130Phys_Rev_D.pdf
", "abstract": "We present the first modeled search for gravitational waves using the complete binary black-hole gravitational waveform from inspiral through the merger and ringdown for binaries with negligible component spin. We searched approximately 2 years of LIGO data, taken between November 2005 and September 2007, for systems with component masses of 1\u201399M_\u2299 and total masses of 25\u2013100M_\u2299. We did not detect any plausible gravitational-wave signals but we do place upper limits on the merger rate of binary black holes as a function of the component masses in this range. We constrain the rate of mergers for 19M_\u2299 \u2264 m_1, m_2 \u2264 28M_\u2299 binary black-hole systems with negligible spin to be no more than 2.0\u2009\u2009Mpc^(-3)\u2009Myr^(-1) at 90% confidence.", "date": "2011-06-06", "date_type": "published", "publication": "Physical Review D", "volume": "83", "number": "12", "publisher": "American Physical Society", "pagerange": "Art. No. 122005", "id_number": "CaltechAUTHORS:20110620-080921042", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110620-080921042", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.83.122005", "primary_object": { "basename": "Abadie2011p14130Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/32x62-3re57/files/Abadie2011p14130Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2011", "author_list": "Abbott, B. P.; Abadie, J.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/p2tew-bh859", "eprint_id": 21741, "eprint_status": "archive", "datestamp": "2023-08-19 04:41:25", "lastmod": "2023-10-21 00:17:20", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mak-C", "name": { "family": "Mak", "given": "C." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McClelland-D-E", "name": { "family": "McClelland", "given": "D. E." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mitra-S", "name": { "family": "Mitra", "given": "S." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Somiya-K", "name": { "family": "Somiya", "given": "K." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A-E", "name": { "family": "Villar", "given": "A. E." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Calibration of the LIGO gravitational wave detectors in the fifth science run", "ispublished": "pub", "full_text_status": "restricted", "keywords": "Interferometer, Calibration, Control systems, Gravitational waves", "note": "\u00a9 2010 Elsevier B.V. Received 23 July 2010, Accepted 28 July 2010, Available online 10 August 2010. The authors gratefully acknowledge the support of the United\nStates National Science Foundation for the construction and\noperation of the LIGO Laboratory and the Science and Technology\nFacilities Council of the United Kingdom, the Max-Planck-Society,\nand the State of Niedersachsen/Germany for support of the\nconstruction and operation of the GEO600 detector. The authors\nalso gratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the Council of\nScientific and Industrial Research of India, the Istituto Nazionale\ndi Fisica Nucleare of Italy, the Spanish Ministerio de Educacion y\nCiencia, the Conselleria d'Economia Hisendai Innovacio of the\nGovern de les Illes Balears, the Royal Society, the Scottish Funding\nCouncil, the Scottish Universities Physics Alliance, The National\nAeronautics and Space Administration, the Carnegie Trust, the\nLeverhulme Trust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan Foundation.\nLIGO was constructed by the California Institute of Technology\nand Massachusetts Institute of Technology with funding from the\nNational Science Foundation and operates under cooperative\nagreement PHY-0107417. This paper has LIGO Document Number\nLIGO-P0900120.", "abstract": "The Laser Interferometer Gravitational Wave Observatory (LIGO) is a network of three detectors built to detect local perturbations in the space-time metric from astrophysical sources These detectors two in Hanford WA and one in Livingston LA are power-recycled Fabry-Perot Michelson interferometers In their fifth science run (S5) between November 2005 and October 2007 these detectors accumulated one year of triple coincident data while operating at their designed sensitivity In this paper we describe the calibration of the instruments in the S5 data set including measurement techniques and uncertainty estimation.", "date": "2010-12-01", "date_type": "published", "publication": "Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment", "volume": "624", "number": "1", "publisher": "Elsevier", "pagerange": "223-240", "id_number": "CaltechAUTHORS:20110112-154537740", "issn": "0168-9002", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110112-154537740", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "Conselleria d Economia Hisenda i Innovacio of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Caltech" }, { "agency": "Massachusetts Institute of Technology (MIT)" }, { "agency": "NSF", "grant_number": "PHY-0107417" }, { "agency": "Scottish Universities Physics Alliance" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P0900120", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "doi": "10.1016/j.nima.2010.07.089", "resource_type": "article", "pub_year": "2010", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/1hy59-nd388", "eprint_id": 21618, "eprint_status": "archive", "datestamp": "2023-08-19 04:22:15", "lastmod": "2023-10-21 00:11:16", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. 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P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Aronsson-M", "name": { "family": "Aronsson", "given": "M." } }, { "id": "Aso-Y", "name": { "family": "Aso", "given": "Y." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cannon-K-C", "name": { "family": "Cannon", "given": "K. C." }, "orcid": "0000-0003-4068-6572" }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Dannenberg-R", "name": { "family": "Dannenberg", "given": "R." } }, { "id": "Daudert-B", "name": { "family": "Daudert", "given": "B." } }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Driggers-J-C", "name": { "family": "Driggers", "given": "J. C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Engel-R", "name": { "family": "Engel", "given": "R." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A", "name": { "family": "Heptonstall", "given": "A." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mak-C", "name": { "family": "Mak", "given": "C." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mitra-S", "name": { "family": "Mitra", "given": "S." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Turner-L", "name": { "family": "Turner", "given": "L." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for gravitational waves from compact binary coalescence in LIGO and Virgo data from S5 and VSR1", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2010 The American Physical Society.\nReceived 25 June 2010; published 5 November 2010.\n\nThe authors gratefully acknowledge the support of\nthe United States National Science Foundation for the\nconstruction and operation of the LIGO Laboratory, the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector, and the Italian\nIstituto Nazionale di Fisica Nucleare and the French\nCentre National de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors\nalso gratefully acknowledge the support of the research by\nthese agencies and by the Australian Research Council, the\nCouncil of Scientific and Industrial Research of India, the\nIstituto Nazionale di Fisica Nucleare of Italy, the Spanish\nMinisterio de Educacio\u00b4n y Ciencia, the Conselleria\nd'Economia Hisenda i Innovacio\u00b4 of the Govern de les Illes\nBalears, the Foundation for Fundamental Research on\nMatter supported by the Netherlands Organisation for\nScientific Research, the Polish Ministry of Science and\nHigher Education, the FOCUS Programme of Foundation\nfor Polish Science, the Royal Society, the Scottish Funding\nCouncil, the Scottish Universities Physics Alliance, The\nNational Aeronautics and Space Administration, the\nCarnegie Trust, the Leverhulme Trust, the David and\nLucile Packard Foundation, the Research Corporation, and\nthe Alfred P. Sloan Foundation. This document has been\nassigned LIGO Laboratory document number P0900305-v6.\n\nPublished - Abadie2010p11996Phys_Rev_D.pdf
", "abstract": "We report the results of the first search for gravitational waves from compact binary coalescence using data from the Laser Interferometer Gravitational-Wave Observatory and Virgo detectors. Five months of data were collected during the Laser Interferometer Gravitational-Wave Observatory's S5 and Virgo's VSR1 science runs. The search focused on signals from binary mergers with a total mass between 2 and 35M_\u2299. No gravitational waves are identified. The cumulative 90%-confidence upper limits on the rate of compact binary coalescence are calculated for nonspinning binary neutron stars, black hole-neutron star systems, and binary black holes to be 8.7\u00d710^(-3)\u2009\u2009yr^(-1)\u2009L_(10)^(-1), 2.2\u00d710^(-3)\u2009\u2009yr^(-1)\u2009L_(10)^(-1), and 4.4\u00d710^(-4)\u2009\u2009yr^(-1)\u2009L_(10)^(-1), respectively, where L_(10) is 10^(10) times the blue solar luminosity. These upper limits are compared with astrophysical expectations.", "date": "2010-11-05", "date_type": "published", "publication": "Physical Review D", "volume": "82", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102001", "id_number": "CaltechAUTHORS:20110106-093745583", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110106-093745583", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "P0900305-v6", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.82.102001", "primary_object": { "basename": "Abadie2010p11996Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/1hy59-nd388/files/Abadie2010p11996Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2010", "author_list": "Abadie, J.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/axxa0-gtw42", "eprint_id": 21180, "eprint_status": "archive", "datestamp": "2023-09-18 15:25:06", "lastmod": "2023-10-23 22:33:18", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Aronsson-M", "name": { "family": "Aronsson", "given": "M." } }, { "id": "Aso-Y", "name": { "family": "Aso", "given": "Y." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boyle-M", "name": { "family": "Boyle", "given": "M." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cannon-K-C", "name": { "family": "Cannon", "given": "K. C." }, "orcid": "0000-0003-4068-6572" }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Yanbei" }, "orcid": "0000-0002-9730-9463" }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Dannenberg-R", "name": { "family": "Dannenberg", "given": "R." } }, { "id": "Daudert-B", "name": { "family": "Daudert", "given": "B." } }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Driggers-J-C", "name": { "family": "Driggers", "given": "J. C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Engel-R", "name": { "family": "Engel", "given": "R." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A", "name": { "family": "Heptonstall", "given": "A." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mak-C", "name": { "family": "Mak", "given": "C." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mino-", "name": { "family": "Mino", "given": "Y." } }, { "id": "Mitra-S", "name": { "family": "Mitra", "given": "S." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "First search for gravitational waves from the youngest known neutron star", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves, stars: neutron, supernovae: individual (Cassiopeia A)", "note": "\u00a9 2010 American Astronomical Society. Received 2010 June 30; accepted 2010 August 21; published 2010 September 30. The authors gratefully acknowledge the support of the United\nStates National Science Foundation for the construction and operation\nof the LIGO Laboratory and the Science and Technology\nFacilities Council of the United Kingdom, the Max-Planck-\nSociety, and the State of Niedersachsen/Germany for support\nof the construction and operation of the GEO600 detector. The\nauthors also gratefully acknowledge the support of the research\nby these agencies and by the Australian Research Council, the\nCouncil of Scientific and Industrial Research of India, the Istituto\nNazionale di FisicaNucleare of Italy, the Spanish Ministerio\nde Educaci\u00b4on y Ciencia, the Conselleria d'Economia, Hisenda\ni Innovaci\u00b4o of the Govern de les Illes Balears, the Royal Society,\nthe Scottish Funding Council, the Scottish Universities\nPhysics Alliance, The National Aeronautics and Space Administration,\nthe Carnegie Trust, the Leverhulme Trust, the David\nand Lucile Packard Foundation, the Research Corporation, and\nthe Alfred P. Sloan Foundation. This paper has been designated\nLIGO Document No. LIGO-P1000028-v7.\n\nPublished - Abadie2010p12052Astrophys_J.pdf
", "abstract": "We present a search for periodic gravitational waves from the neutron star in the supernova remnant Cassiopeia\nA. The search coherently analyzes data in a 12 day interval taken from the fifth science run of the Laser\nInterferometer Gravitational-Wave Observatory. It searches gravitational-wave frequencies from 100 to 300 Hz\nand covers a wide range of first and second frequency derivatives appropriate for the age of the remnant and\nfor different spin-down mechanisms. No gravitational-wave signal was detected. Within the range of search\nfrequencies, we set 95% confidence upper limits of (0.7\u20131.2) \u00d7 10^(\u221224) on the intrinsic gravitational-wave\nstrain, (0.4\u20134) \u00d7 10^(\u22124) on the equatorial ellipticity of the neutron star, and 0.005\u20130.14 on the amplitude of\nr-mode oscillations of the neutron star. These direct upper limits beat indirect limits derived from energy\nconservation and enter the range of theoretical predictions involving crystalline exotic matter or runaway r-modes.\nThis paper is also the first gravitational-wave search to present upper limits on the r-mode amplitude.", "date": "2010-10-20", "date_type": "published", "publication": "Astrophysical Journal", "volume": "722", "number": "2", "publisher": "American Astronomical Society", "pagerange": "1504-1513", "id_number": "CaltechAUTHORS:20101206-105405445", "issn": "0004-637X", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20101206-105405445", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "doi": "10.1088/0004-637X/722/2/1504", "primary_object": { "basename": "Abadie2010p12052Astrophys_J.pdf", "url": "https://authors.library.caltech.edu/records/axxa0-gtw42/files/Abadie2010p12052Astrophys_J.pdf" }, "resource_type": "article", "pub_year": "2010", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/fdmtf-4f105", "eprint_id": 19824, "eprint_status": "archive", "datestamp": "2023-08-19 03:52:18", "lastmod": "2023-10-20 21:56:12", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Cohen-M-I", "name": { "family": "Cohen", "given": "Michael I." } }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "Curt" } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Searches for cosmic-string gravitational-wave bursts in Mock LISA Data", "ispublished": "pub", "full_text_status": "restricted", "note": "\u00a9 2010 IOP Publishing Ltd.\n\nReceived 22 February 2010, in final form 6 July 2010.\nPublished 29 July 2010.\n\nThis research relied crucially on the hard work of the developers of open-source scientific\nsoftware: we thank the authors and maintainers the of NumPy and SciPy Python libraries, and\nespecially F Feroz and colleagues (MultiNest) and C Fonnesbeck and colleagues (PyMC).We\nthank J Gair, N Cornish and J Shapiro Key for useful interactions. The numerical computation\nfor this work was performed primarily with computing resources from the Caltech Center for\nAdvanced Computing Research. Much of the research described in this paper was carried\nout at the Jet Propulsion Laboratory, California Institute of Technology, under a contract\nwith the National Aeronautics and Space Administration. MC, CC and MV also gratefully\nacknowledge support from the NASA grant NNX07AM80G.", "abstract": "A network of observable, macroscopic cosmic (super-)strings may well have\nformed in the early Universe. If so, the cusps that generically develop\non cosmic-string loops emit bursts of gravitational radiation that could be\ndetectable by gravitational-wave interferometers, such as the ground-based\nLIGO/Virgo detectors and the planned, space-based LISA detector. Here we\nreport on two versions of a LISA-oriented string-burst search pipeline that\nwe have developed and tested within the context of the Mock LISA Data\nChallenges. The two versions rely on the publicly available MultiNest and\nPyMC software packages, respectively. To reduce the effective dimensionality\nof the search space, our implementations use the F-statistic to analytically\nmaximize over the signal's amplitude and polarization, A and \u03c8, and use\nthe FFT to search quickly over burst arrival times t_C. The standard F-statistic\nis essentially a frequentist statistic that maximizes the likelihood;\nwe also demonstrate an approximate, Bayesian version of the F-statistic that\nincorporates realistic priors on A and \u03c8. We calculate how accurately LISA can\nexpect to measure the physical parameters of string-burst sources, and compare\nto results based on the Fisher-matrix approximation. To understand LISA's\nangular resolution for string-burst sources, we draw maps of the waveform\nfitting factor (maximized over (A, \u03c8, t_C)) as a function of the sky position;\nthese maps dramatically illustrate why (for LISA) inferring the correct sky\nlocation of the emitting string loop will often be practically impossible. In\naddition, we identify and elucidate several symmetries that are imbedded in\nthis search problem, and we derive the distribution of cut-off frequencies f_(max)\nfor observable bursts.", "date": "2010-09-21", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "27", "number": "18", "publisher": "IOP", "pagerange": "Art. No. 185012", "id_number": "CaltechAUTHORS:20100908-093644724", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100908-093644724", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NASA", "grant_number": "NNX07AM80G" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/27/18/185012", "resource_type": "article", "pub_year": "2010", "author_list": "Cohen, Michael I.; Cutler, Curt; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/baaxv-43k56", "eprint_id": 19399, "eprint_status": "archive", "datestamp": "2023-08-19 03:46:26", "lastmod": "2023-10-20 20:39:19", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Aronsson-M", "name": { "family": "Aronsson", "given": "M." } }, { "id": "Aso-Y", "name": { "family": "Aso", "given": "Y." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cannon-K-C", "name": { "family": "Cannon", "given": "K. C." }, "orcid": "0000-0003-4068-6572" }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Dannenberg-R", "name": { "family": "Dannenberg", "given": "R." } }, { "id": "Daudert-B", "name": { "family": "Daudert", "given": "B." } }, { "id": "Dergachev-V", "name": { "family": "Dergachev", "given": "V." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Driggers-J-C", "name": { "family": "Driggers", "given": "J. C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Engel-R", "name": { "family": "Engel", "given": "R." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A", "name": { "family": "Heptonstall", "given": "A." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mak-C", "name": { "family": "Mak", "given": "C." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mitra-S", "name": { "family": "Mitra", "given": "S." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Osthelder-C", "name": { "family": "Osthelder", "given": "C." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Privitera-S", "name": { "family": "Privitera", "given": "S." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Singer-A", "name": { "family": "Singer", "given": "A." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Boyle-M", "name": { "family": "Boyle", "given": "M." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Yanbei" }, "orcid": "0000-0002-9730-9463" }, { "id": "Luan-J", "name": { "family": "Luan", "given": "J." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors", "ispublished": "pub", "full_text_status": "restricted", "note": "\u00a9 2010 IOP Publishing Ltd.\nReceived 26 March 2010, in final form 15 May 2010.\nPublished 16 July 2010.\n\nThe authors gratefully acknowledge the support of the United States National Science\nFoundation for the construction and operation of the LIGO Laboratory, the Science and\nTechnology Facilities Council of the United Kingdom, the Max-Planck-Society, the State\nof Niedersachsen/Germany for support of the construction and operation of the GEO600\ndetector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National\nde la Recherche Scientifique for the construction and operation of the Virgo detector. The\nauthors also gratefully acknowledge the support of the research by these agencies and by\nthe Australian Research Council, the Council of Scientific and Industrial Research of India,\nthe Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u00f3n y\nCiencia, the Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the\nFoundation for Fundamental Research on Matter supported by the Netherlands Organisation\nfor Scientific Research, the Polish Ministry of Science and Higher Education, the FOCUS\nProgramme of Foundation for Polish Science, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space\nAdministration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation and the Alfred P Sloan Foundation. One of us (CK)\nwould like to acknowledge the European Commission.", "abstract": "We present an up-to-date, comprehensive summary of the rates for all types\nof compact binary coalescence sources detectable by the initial and advanced\nversions of the ground-based gravitational-wave detectors LIGO and Virgo.\nAstrophysical estimates for compact-binary coalescence rates depend on a\nnumber of assumptions and unknown model parameters and are still uncertain.\nThemost confident among these estimates are the rate predictions for coalescing\nbinary neutron stars which are based on extrapolations from observed binary\npulsars in our galaxy. These yield a likely coalescence rate of 100 Myr^(\u22121)\nper Milky Way Equivalent Galaxy (MWEG), although the rate could plausibly\nrange from 1 Myr^(\u22121) MWEG^(\u22121) to 1000 Myr^(\u22121) MWEG^(\u22121) (Kalogera et al 2004\nAstrophys. J. 601 L179; Kalogera et al 2004 Astrophys. J. 614 L137 (erratum)).\nWe convert coalescence rates into detection rates based on data from the LIGO\nS5 and Virgo VSR2 science runs and projected sensitivities for our advanced\ndetectors. Using the detector sensitivities derived from these data, we find a\nlikely detection rate of 0.02 per year for Initial LIGO\u2013Virgo interferometers,\nwith a plausible range between 2 \u00d7 10^(\u22124) and 0.2 per year. The likely binary\nneutron\u2013star detection rate for the Advanced LIGO\u2013Virgo network increases\nto 40 events per year, with a range between 0.4 and 400 per year.", "date": "2010-09-07", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "27", "number": "17", "publisher": "IOP", "pagerange": "Art. No. 173001", "id_number": "CaltechAUTHORS:20100811-144535085", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100811-144535085", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P Sloan Foundation" }, { "agency": "European Commission" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1088/0264-9381/27/17/173001", "resource_type": "article", "pub_year": "2010", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/nfwzd-ewj40", "eprint_id": 18635, "eprint_status": "archive", "datestamp": "2023-08-22 00:03:42", "lastmod": "2023-10-20 16:36:55", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Aso-Y", "name": { "family": "Aso", "given": "Y." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barton-M-A", "name": { "family": "Barton", "given": "M. A." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cannon-K-C", "name": { "family": "Cannon", "given": "K. C." }, "orcid": "0000-0003-4068-6572" }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Daudert-B", "name": { "family": "Daudert", "given": "B." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Echols-C", "name": { "family": "Echols", "given": "C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A", "name": { "family": "Heptonstall", "given": "A." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Li-C", "name": { "family": "Li", "given": "C." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C", "name": { "family": "Torrie", "given": "C." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search For Gravitational-wave Bursts Associated with Gamma-ray Bursts using Data from LIGO Science Run 5 and Virgo Science Run 1", "ispublished": "pub", "full_text_status": "public", "keywords": "gamma rays: bursts: general; gravitational waves", "note": "\u00a9 2010 The American Astronomical Society. Received 2009 September 15; accepted 2010 March 8; published 2010 May 12. We are indebted to the observers of the electromagnetic events\nand the GCN for providing us with valuable data. The authors\ngratefully acknowledge the support of the United States National\nScience Foundation for the construction and operation\nof the LIGO Laboratory, the Science and Technology Facilities\nCouncil of the United Kingdom, the Max-Planck-Society, and\nthe State of Niedersachsen/Germany for support of the construction\nand operation of the GEO600 detector, and the Italian\nIstituto Nazionale di Fisica Nucleare and the French Centre\nNational de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors also gratefully\nacknowledge research support by these agencies and by\nthe Australian Research Council, the Council of Scientific and\nIndustrial Research of India, the Istituto Nazionale di Fisica Nucleare\nof Italy, the Spanish Ministerio de Educaci\u00b4on y Ciencia,\nthe Conselleria d'Economia Hisenda i Innovaci\u00b4o of the Govern\nde les Illes Balears, the Foundation for Fundamental Research\non Matter supported by the Netherlands Organisation for Scientific\nResearch, the Royal Society, the Scottish Funding Council,\nthe Scottish Universities Physics Alliance, The National\nAeronautics and Space Administration, the Carnegie Trust, the\nLeverhulme Trust, the David and Lucile Packard Foundation,\nthe Research Corporation, and the Alfred P. Sloan Foundation.\nThis document has been assigned LIGO Laboratory document\nnumber LIGO-P0900023-v16.\n\nPublished - Abbott2010p10222Astrophys_J.pdf
", "abstract": "We present the results of a search for gravitational-wave bursts (GWBs) associated with 137 gamma-ray bursts (GRBs) that were detected by satellite-based gamma-ray experiments during the fifth LIGO science run and first Virgo science run. The data used in this analysis were collected from 2005 November 4 to 2007 October 1, and most of the GRB triggers were from the Swift satellite. The search uses a coherent network analysis method that takes into account the different locations and orientations of the interferometers at the three LIGO-Virgo sites. We find no evidence for GWB signals associated with this sample of GRBs. Using simulated short-duration (<1 s) waveforms, we set upper limits on the amplitude of gravitational waves associated with each GRB. We also place lower bounds on the distance to each GRB under the assumption of a fixed energy emission in gravitational waves, with a median limit of D ~ 12 Mpc(E^(iso)_(GW)/0.01 M_\u2609 c ^(2)^(1/2) for emission at frequencies around 150 Hz, where the LIGO-Virgo detector network has best sensitivity. We present astrophysical interpretations and implications of these results, and prospects for corresponding searches during future LIGO-Virgo runs.", "date": "2010-06-01", "date_type": "published", "publication": "Astrophysical Journal", "volume": "715", "number": "2", "publisher": "American Astronomical Society", "pagerange": "1438-1452", "id_number": "CaltechAUTHORS:20100610-092615176", "issn": "0004-637X", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100610-092615176", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P0900023-v16", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1088/0004-637X/715/2/1438", "primary_object": { "basename": "Abbott2010p10222Astrophys_J.pdf", "url": "https://authors.library.caltech.edu/records/nfwzd-ewj40/files/Abbott2010p10222Astrophys_J.pdf" }, "resource_type": "article", "pub_year": "2010", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/gztj1-fh171", "eprint_id": 18621, "eprint_status": "archive", "datestamp": "2023-08-22 00:03:01", "lastmod": "2023-10-20 16:36:15", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Aso-Y", "name": { "family": "Aso", "given": "Y." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cannon-K-C", "name": { "family": "Cannon", "given": "K. C." }, "orcid": "0000-0003-4068-6572" }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Daudert-B", "name": { "family": "Daudert", "given": "B." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Driggers-J", "name": { "family": "Driggers", "given": "J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A", "name": { "family": "Heptonstall", "given": "A." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. J." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mak-C", "name": { "family": "Mak", "given": "C." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Mitra-S", "name": { "family": "Mitra", "given": "S." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Smith-S-R", "name": { "family": "Smith", "given": "S. R." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Turner-L", "name": { "family": "Turner", "given": "L." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for Gravitational-wave Inspiral Signals Associated with Short Gamma-ray Bursts During LIGO's Fifth and Virgo's First Science Run", "ispublished": "pub", "full_text_status": "public", "keywords": "binaries: close; gamma-ray burst: general; gravitational waves", "note": "\u00a9 2010 The American Astronomical Society. \nReceived 2010 January 18; accepted 2010 March 6; published 2010 May 12. We are indebted to the observers of the electromagnetic events\nand the GCN for providing us with valuable data. The authors\ngratefully acknowledge the support of the United States National\nScience Foundation for the construction and operation\nof the LIGO Laboratory, the Science and Technology Facilities\nCouncil of the United Kingdom, the Max-Planck-Society, and\nthe State of Niedersachsen/Germany for support of the construction\nand operation of the GEO600 detector, and the Italian\nIstituto Nazionale di Fisica Nucleare and the French Centre\nNational de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors also gratefully\nacknowledge research support by these agencies and by\nthe Australian Research Council, the Council of Scientific and\nIndustrial Research of India, the Istituto Nazionale di Fisica Nucleare\nof Italy, the Spanish Ministerio de Educaci\u00b4on y Ciencia,\nthe Conselleria d'Economia Hisenda i Innovaci\u00b4o of the Govern\nde les Illes Balears, the Foundation for Fundamental Research\non Matter supported by the Netherlands Organisation for Scientific\nResearch, the Royal Society, the Scottish Funding Council,\nthe Scottish Universities Physics Alliance, The National Aeronautics\nand Space Administration, the Carnegie Trust, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan Foundation.\n\nThis document bears the LIGO document number P0900074.\n\nPublished - Abadie2010p10218Astrophys_J.pdf
", "abstract": "Progenitor scenarios for short gamma-ray bursts (short GRBs) include coalescenses of two neutron stars or a neutron star and black hole, which would necessarily be accompanied by the emission of strong gravitational waves. We present a search for these known gravitational-wave signatures in temporal and directional coincidence with 22 GRBs that had sufficient gravitational-wave data available in multiple instruments during LIGO's fifth science run, S5, and Virgo's first science run, VSR1. We find no statistically significant gravitational-wave candidates within a [ \u2013 5, + 1) s window around the trigger time of any GRB. Using the Wilcoxon-Mann-Whitney U-test, we find no evidence for an excess of weak gravitational-wave signals in our sample of GRBs. We exclude neutron star-black hole progenitors to a median 90% confidence exclusion distance of 6.7 Mpc.", "date": "2010-06-01", "date_type": "published", "publication": "Astrophysical Journal", "volume": "715", "number": "2", "publisher": "American Astronomical Society", "pagerange": "1453-1461", "id_number": "CaltechAUTHORS:20100609-133535106", "issn": "0004-637X", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100609-133535106", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovacio of the Govern de les Illes Balears" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "P0900074", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1088/0004-637X/715/2/1453", "primary_object": { "basename": "Abadie2010p10218Astrophys_J.pdf", "url": "https://authors.library.caltech.edu/records/gztj1-fh171/files/Abadie2010p10218Astrophys_J.pdf" }, "resource_type": "article", "pub_year": "2010", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/cs5ya-axb14", "eprint_id": 18796, "eprint_status": "archive", "datestamp": "2023-08-19 02:30:08", "lastmod": "2023-10-20 16:46:45", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abadie-J", "name": { "family": "Abadie", "given": "J." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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P." } }, { "id": "Driggers-J", "name": { "family": "Driggers", "given": "J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A", "name": { "family": "Heptonstall", "given": "A." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P-J", "name": { "family": "King", "given": "P. 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N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Mitra-S", "name": { "family": "Mitra", "given": "S." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Seifert-F", "name": { "family": "Seifert", "given": "F." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Somiya-K", "name": { "family": "Somiya", "given": "K." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C-I", "name": { "family": "Torrie", "given": "C. I." } }, { "id": "Turner-L", "name": { "family": "Turner", "given": "L." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yeaton-Massey-D", "name": { "family": "Yeaton-Massey", "given": "D." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "All-sky search for gravitational-wave bursts in the first joint LIGO-GEO-Virgo run", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2010 The American Physical Society. \n\nReceived 4 March 2010; published 5 May 2010. \n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory, the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO 600 detector, and the Italian\nIstituto Nazionale di Fisica Nucleare and the French Centre\nNational de la Recherche Scientifique for the construction\nand operation of the Virgo detector. The authors also gratefully\nacknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nCouncil of Scientific and Industrial Research of India,\nthe Istituto Nazionale di Fisica Nucleare of Italy, the\nSpanish Ministerio de Educaci\u03ccn y Ciencia, the\nConselleria d'Economia Hisenda i Innovaci\u03cc of the\nGovern de les Illes Balears, the Foundation for\nFundamental Research on Matter supported by the\nNetherlands Organisation for Scientific Research, the\nPolish Ministry of Science and Higher Education, the\nFOCUS Programme of Foundation for Polish Science,\nthe Royal Society, the Scottish Funding Council, the\nScottish Universities Physics Alliance, the National\nAeronautics and Space Administration, the Carnegie\nTrust, the Leverhulme Trust, the David and Lucile\nPackard Foundation, the Research Corporation, and the\nAlfred P. Sloan Foundation. This document has been assigned\nLIGO Laboratory document number LIGOP0900108-\nv6.\n\nPublished - Abadie2010p10413Phys_Rev_D.pdf
", "abstract": "We present results from an all-sky search for unmodeled gravitational-wave bursts in the data collected by the LIGO, GEO 600 and Virgo detectors between November 2006 and October 2007. The search is performed by three different analysis algorithms over the frequency band 50\u20136000 Hz. Data are analyzed for times with at least two of the four LIGO-Virgo detectors in coincident operation, with a total live time of 266 days. No events produced by the search algorithms survive the selection cuts. We set a frequentist upper limit on the rate of gravitational-wave bursts impinging on our network of detectors. When combined with the previous LIGO search of the data collected between November 2005 and November 2006, the upper limit on the rate of detectable gravitational-wave bursts in the 64\u20132048 Hz band is 2.0 events per year at 90% confidence. We also present event rate versus strength exclusion plots for several types of plausible burst waveforms. The sensitivity of the combined search is expressed in terms of the root-sum-squared strain amplitude for a variety of simulated waveforms and lies in the range 6\u00d710^(-22)\u2009\u2009Hz^(-1/2) to 2\u00d710^(-20)\u2009\u2009Hz^(-1/2). This is the first untriggered burst search to use data from the LIGO and Virgo detectors together, and the most sensitive untriggered burst search performed so far.", "date": "2010-05-05", "date_type": "published", "publication": "Physical Review D", "volume": "81", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102001", "id_number": "CaltechAUTHORS:20100624-112258931", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100624-112258931", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Nederlandse Organisatie voor Wetenschappelijk Onderzoek (NWO)" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "collection": "CaltechAUTHORS", "other_numbering_system": { "items": [ { "id": "P0900108-v6", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR", "value": "TAPIR" }, { "id": "LIGO", "value": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1103/PhysRevD.81.102001", "primary_object": { "basename": "Abadie2010p10413Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/cs5ya-axb14/files/Abadie2010p10413Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2010", "author_list": "Abadie, J.; Abbott, B. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/y8qbw-f1968", "eprint_id": 20469, "eprint_status": "archive", "datestamp": "2023-08-19 02:16:46", "lastmod": "2023-10-20 23:05:12", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Babak-S", "name": { "family": "Babak", "given": "Stanislav" } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" }, { "id": "Cohen-Michael", "name": { "family": "Cohen", "given": "Michael" } }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "Curt" } } ] }, "title": "The Mock LISA Data Challenges: from challenge 3 to challenge 4", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2010 IOP Publishing Ltd.\nReceived 16 November 2009, in final form 26 January 2010.\nPublished 6 April 2010.\n\nThe authors acknowledge support from the German Aerospace Center (SB, AP, JTW); the Max-Planck Society (SB, JTW, AP, RP, ELR); the LISA Mission Science Office at JPL (CC, MV); MNiSW grant N N203 387237 (AB, AK); NASA grants NNG04GD52G (MB), NNG05GI69G and NNX07AJ61G (NJC), 06-BEFS06-31 (MV and CC), NNX07AH22G (IM), and the NASA Center for GW Astronomy at the University of Texas, Brownsville; NSF grant PHY-0855494 (JTW), and the NSF A&A postdoctoral fellowship under AST- 0901985 (IM); the Science and Technology Facilities Council (AV); St Catharine's College, Cambridge (JG); E.U. FEDER funds, Spanish Ministerio de Ciencia e Innovaci\u00f3n projects FPA2007-60220, HA2007-0042 and CSD2007-00042, Govern de les Illes Balears, Conselleria d'Economia, Hisenda i Innovaci\u00f3 (MT). CC's and MV's work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.\n\nPublished - Babak2010p11567Classical_Quant_Grav.pdf
", "abstract": "The Mock LISA Data Challenges are a program to demonstrate LISA data-analysis capabilities and to encourage their development. Each round of challenges consists of one or more datasets containing simulated instrument noise and gravitational waves from sources of undisclosed parameters. Participants analyze the datasets and report best-fit solutions for the source parameters. Here we present the results of the third challenge, issued in April 2008, which demonstrated the positive recovery of signals from chirping galactic binaries, from spinning supermassive-black-hole binaries (with optimal SNRs between ~10 and 2000), from simultaneous extreme-mass-ratio inspirals (SNRs of 10\u201350), from cosmic-string-cusp bursts (SNRs of 10\u2013100), and from a relatively loud isotropic background with \u03a9_(gw)(f) ~ 10^(\u221211), slightly below the LISA instrument noise.", "date": "2010-04-21", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "27", "number": "8", "publisher": "IOP", "pagerange": "Art. No. 084009", "id_number": "CaltechAUTHORS:20101021-130719200", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20101021-130719200", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "German Aerospace Center" }, { "agency": "Max-Planck Society" }, { "agency": "JPL LISA Mission Science Office" }, { "agency": "Minister nauki i szkolnictwa wy\u017cszego (MNiSW)", "grant_number": "N N203 387237" }, { "agency": "NASA", "grant_number": "NNG04GD52G" }, { "agency": "NASA", "grant_number": "NNG05GI69G" }, { "agency": "NASA", "grant_number": "NNX07AJ61G" }, { "agency": "NASA", "grant_number": "06-BEFS06-31" }, { "agency": "NASA", "grant_number": "NNX07AH22G" }, { "agency": "University of Texas NASA Center for GW Astronomy" }, { "agency": "NSF", "grant_number": "PHY-0855494" }, { "agency": "NSF A&A postdoctoral fellowship", "grant_number": "AST- 0901985" }, { "agency": "Science and Technology Facilities Council" }, { "agency": "St Catharine's College, Cambridge" }, { "agency": "European Union (EU) FEDER" }, { "agency": "Spanish Ministerio de Ciencia e Innovaci\u00f3n", "grant_number": "FPA2007-60220" }, { "agency": "Spanish Ministerio de Ciencia e Innovaci\u00f3n", "grant_number": "HA2007-0042" }, { "agency": "Spanish Ministerio de Ciencia e Innovaci\u00f3n", "grant_number": "CSD2007-00042" }, { "agency": "Govern de les Illes Balears, Conselleria d'Economia, Hisenda i Innovaci\u00f3" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/27/8/084009", "primary_object": { "basename": "Babak2010p11567Classical_Quant_Grav.pdf", "url": "https://authors.library.caltech.edu/records/y8qbw-f1968/files/Babak2010p11567Classical_Quant_Grav.pdf" }, "resource_type": "article", "pub_year": "2010", "author_list": "Babak, Stanislav; Vallisneri, Michele; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/g6vzh-qb331", "eprint_id": 85214, "eprint_status": "archive", "datestamp": "2023-08-21 23:44:28", "lastmod": "2023-10-18 17:58:36", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R." }, "orcid": "0000-0002-5731-5076" }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Aso-Y", "name": { "family": "Aso", "given": "Y." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barton-M-A", "name": { "family": "Barton", "given": "M. A." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-J-K", "name": { "family": "Blackburn", "given": "J. K." }, "orcid": "0000-0002-3838-2986" }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Brooks-A-F", "name": { "family": "Brooks", "given": "A. F." }, "orcid": "0000-0003-4295-792X" }, { "id": "Cannon-K-C", "name": { "family": "Cannon", "given": "K. C." }, "orcid": "0000-0003-4068-6572" }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chalermsongsak-T", "name": { "family": "Chalermsongsak", "given": "T." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D. C." }, "orcid": "0000-0002-6427-3222" }, { "id": "Daubert-B", "name": { "family": "Daubert", "given": "B." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Echols-C", "name": { "family": "Echols", "given": "C." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Gustafson-E-K", "name": { "family": "Gustafson", "given": "E. K." } }, { "id": "Hanna-C", "name": { "family": "Hanna", "given": "C." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Heptonstall-A", "name": { "family": "Heptonstall", "given": "A." } }, { "id": "Hodge-K-A", "name": { "family": "Hodge", "given": "K. A." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kalmus-P", "name": { "family": "Kalmus", "given": "P." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P. E." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "McIntyre-G", "name": { "family": "McIntyre", "given": "G." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Ogin-G-H", "name": { "family": "Ogin", "given": "G. H." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Searle-A-C", "name": { "family": "Searle", "given": "A. C." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Sengupta-A-S", "name": { "family": "Sengupta", "given": "A. S." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Stochino-A", "name": { "family": "Stochino", "given": "A." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Torrie-C", "name": { "family": "Torrie", "given": "C." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R-L", "name": { "family": "Ward", "given": "R. L." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Li-C", "name": { "family": "Li", "given": "C." } }, { "id": "Mino-Y", "name": { "family": "Mino", "given": "Y." } }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Somiya-Kentaro", "name": { "family": "Somiya", "given": "K." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } } ] }, "title": "Searches for gravitational waves from known pulsars with S5 LIGO data", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; pulsars: general", "note": "\u00a9 2010 American Astronomical Society. \n\nReceived 2009 October 11. Accepted 2010 February 26. Published 2010 March 24. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u00f3n y Ciencia, the Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears, the Foundation for Fundamental Research on Matter supported by the Netherlands Organisation for Scientific Research, the Royal Society, the Scottish Funding Council, the Polish Ministry of Science and Higher Education, the FOCUS Programme of Foundation for Polish Science, the Scottish Universities Physics Alliance, the National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. LIGO Document No. LIGO-P080112-v5. Pulsar research at UBC is supported by a Natural Sciences and Engineering Research Council of Canada Discovery Grant. The Parkes radio telescope is part of the Australia Telescope which is funded by the Commonwealth Government for operation as a National Facility managed by CSIRO. The National Radio Astronomy Observatory is a facility of the United States National Science Foundation operated under cooperative agreement by Associated Universities, Inc. We thank Maura McLaughlin for useful discussions.\n\nPublished - Abbott_2010_ApJ_713_671.pdf
Submitted - 0909.3583.pdf
", "abstract": "We present a search for gravitational waves from 116 known millisecond and young pulsars using data from the fifth science run of the LIGO detectors. For this search, ephemerides overlapping the run period were obtained for all pulsars using radio and X-ray observations. We demonstrate an updated search method that allows for small uncertainties in the pulsar phase parameters to be included in the search. We report no signal detection from any of the targets and therefore interpret our results as upper limits on the gravitational wave signal strength. The most interesting limits are those for young pulsars. We present updated limits on gravitational radiation from the Crab pulsar, where the measured limit is now a factor of 7 below the spin-down limit. This limits the power radiated via gravitational waves to be less than ~2% of the available spin-down power. For the X-ray pulsar J0537 \u2013 6910 we reach the spin-down limit under the assumption that any gravitational wave signal from it stays phase locked to the X-ray pulses over timing glitches, and for pulsars J1913+1011 and J1952+3252 we are only a factor of a few above the spin-down limit. Of the recycled millisecond pulsars, several of the measured upper limits are only about an order of magnitude above their spin-down limits. For these our best (lowest) upper limit on gravitational wave amplitude is 2.3 \u00d7 10^(\u201326) for J1603 \u2013 7202 and our best (lowest) limit on the inferred pulsar ellipticity is 7.0 \u00d7 10^(\u20138) for J2124 \u2013 3358.", "date": "2010-04-10", "date_type": "published", "publication": "Astrophysical Journal", "volume": "713", "number": "1", "publisher": "American Astronomical Society", "pagerange": "671-685", "id_number": "CaltechAUTHORS:20180309-065629209", "issn": "0004-637X", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180309-065629209", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Centre National de la Recherche Scientifique (CNRS)" }, { "agency": "Australian Research Council" }, { "agency": "Council of Science and Industrial Research (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Stichting voor Fundamenteel Onderzoek der Materie (FOM)" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Ministry of Science and Higher Education (Poland)" }, { "agency": "FOCUS Programme of Foundation for Polish Science" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Commonwealth of Australia" } ] }, "other_numbering_system": { "items": [ { "id": "P080112-v5", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "Virgo Collaboration" ] }, "doi": "10.1088/0004-637X/713/1/671", "primary_object": { "basename": "0909.3583.pdf", "url": "https://authors.library.caltech.edu/records/g6vzh-qb331/files/0909.3583.pdf" }, "related_objects": [ { "basename": "Abbott_2010_ApJ_713_671.pdf", "url": "https://authors.library.caltech.edu/records/g6vzh-qb331/files/Abbott_2010_ApJ_713_671.pdf" } ], "resource_type": "article", "pub_year": "2010", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/gv19a-2pq03", "eprint_id": 18012, "eprint_status": "archive", "datestamp": "2023-08-19 00:34:52", "lastmod": "2023-10-20 15:30:30", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Allen-G", "name": { "family": "Allen", "given": "G." } }, { "id": "Amin-R-S", "name": { "family": "Amin", "given": "R. S." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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E." }, "orcid": "0000-0002-2544-1596" }, { "id": "zur-M\u00fchlen-H", "name": { "family": "zur M\u00fchlen", "given": "H." } }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for high frequency gravitational-wave bursts in the first calendar year of LIGO's fifth science run", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2009 The American Physical Society. \n\nReceived 27 May 2009; published 11 November 2009. T\n\nhe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory, and the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction\nand operation of the GEO 600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nCouncil of Scientific and Industrial Research of India,\nthe Istituto Nazionale di Fisica Nucleare of Italy, the\nSpanish Ministerio de Educacio\u00b4n y Ciencia, the\nConselleria d'Economia Hisenda i Innovacio\u00b4 of the\nGovern de les Illes Balears, the Royal Society, the\nScottish Funding Council, the Scottish Universities\nPhysics Alliance, the National Aeronautics and Space\nAdministration, the Carnegie Trust, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan\nFoundation. The authors thank Luca Baiotti and Luciano\nRezzolla for providing simulation data and valuable discussion\nconcerning the testing of astrophysical waveform\nmodels. This document has been assigned LIGO\nLaboratory document No. LIGO-P080080.\n\nPublished - Abbott2009p6643Phys_Rev_D.pdf
", "abstract": "We present an all-sky search for gravitational waves in the frequency range 1 to 6 kHz during the first calendar year of LIGO's fifth science run. This is the first untriggered LIGO burst analysis to be conducted above 3 kHz. We discuss the unique properties of interferometric data in this regime. 161.3 days of triple-coincident data were analyzed. No gravitational events above threshold were observed and a frequentist upper limit of 5.4\u2009\u2009year^(-1) on the rate of strong gravitational-wave bursts was placed at a 90% confidence level. Implications for specific theoretical models of gravitational-wave emission are also discussed.", "date": "2009-11-15", "date_type": "published", "publication": "Physical Review D", "volume": "80", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102002", "id_number": "CaltechAUTHORS:20100419-091739093", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100419-091739093", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P080080", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.80.102002", "primary_object": { "basename": "Abbott2009p6643Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/gv19a-2pq03/files/Abbott2009p6643Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2009", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/emxnc-44s51", "eprint_id": 17152, "eprint_status": "archive", "datestamp": "2023-08-19 00:34:21", "lastmod": "2023-10-19 22:51:11", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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E." }, "orcid": "0000-0002-2544-1596" }, { "id": "zur-M\u00fchlen-H", "name": { "family": "zur-M\u00fchlen", "given": "H." } }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for gravitational-wave bursts in the first year of the fifth LIGO science run", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2009 The American Physical Society. \n\nReceived 27 May 2009; published 11 November 2009. \n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory and the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen in Germany for support of the construction\nand operation of the GEO600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nCouncil of Scientific and Industrial Research of India,\nthe Istituto Nazionale di Fisica Nucleare of Italy, the\nSpanish Ministerio de Educaci\u03ccn y Ciencia, the\nConselleria d'Economia Hisenda i Innovaci\u03cc of the\nGovern de les Illes Balears, the Royal Society, the\nScottish Funding Council, the Scottish Universities\nPhysics Alliance, the National Aeronautics and Space\nAdministration, the Carnegie Trust, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan\nFoundation. This document has been assigned LIGO\nLaboratory Document No. LIGO-P080056-v12.\n\nPublished - Abbott2009p6632Phys_Rev_D.pdf
", "abstract": "We present the results obtained from an all-sky search for gravitational-wave (GW) bursts in the 64\u2013\n2000 Hz frequency range in data collected by the LIGO detectors during the first year (November 2005\u2014\nNovember 2006) of their fifth science run. The total analyzed live time was 268.6 days. Multiple\nhierarchical data analysis methods were invoked in this search. The overall sensitivity expressed in terms\nof the root-sum-square (rss) strain amplitude h_(rss) for gravitational-wave bursts with various morphologies\nwas in the range of 6 x 10^(-22) Hz^(-1/2) to a few x 10^(-21) Hz^(-1/2). No GW signals were observed and a\nfrequentist upper limit of 3.75 events per year on the rate of strong GW bursts was placed at the 90%\nconfidence level. As in our previous searches, we also combined this rate limit with the detection\nefficiency for selected waveform morphologies to obtain event rate versus strength exclusion curves. In\nsensitivity, these exclusion curves are the most stringent to date.", "date": "2009-11-11", "date_type": "published", "publication": "Physical Review D", "volume": "80", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102001", "id_number": "CaltechAUTHORS:20100112-150144281", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100112-150144281", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "collection": "CaltechAUTHORS", "other_numbering_system": { "items": [ { "id": "LIGO-P080056-v12", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR", "value": "TAPIR" }, { "id": "LIGO", "value": "LIGO" } ] }, "doi": "10.1103/PhysRevD.80.102001", "primary_object": { "basename": "Abbott2009p6632Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/emxnc-44s51/files/Abbott2009p6632Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2009", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/q2zx5-xyq27", "eprint_id": 16433, "eprint_status": "archive", "datestamp": "2023-08-19 00:07:00", "lastmod": "2023-10-19 22:14:01", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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E." }, "orcid": "0000-0002-2544-1596" }, { "id": "zur-M\u00fchlen-H", "name": { "family": "zur-M\u00fchlen", "given": "H." } }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Robinet-F", "name": { "family": "Robinet", "given": "F." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "First LIGO search for gravitational wave bursts from cosmic (super)strings", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2009 The American Physical Society. \n\nReceived 29 May 2009; published 23 September 2009. \n\nThe authors would like to thank Irit Maor and Alexander\nVilenkin for useful discussions. The authors gratefully\nacknowledge the support of the United States National\nScience Foundation for the construction and operation of\nthe LIGO Laboratory and the Particle Physics and\nAstronomy Research Council of the United Kingdom, the\nMax-Planck-Society, and the State of Niedersachsen/\nGermany for support of the construction and operation of\nthe GEO600 detector. The authors also gratefully acknowledge\nthe support of the research by these agencies and by\nthe Australian Research Council, the Natural Sciences and\nEngineering Research Council of Canada, the Council of\nScientific and Industrial Research of India, the Department\nof Science and Technology of India, the Spanish Ministerio\nde Educacion y Ciencia, The National Aeronautics and\nSpace Administration, the John Simon Guggenheim\nFoundation, the Alexander von Humboldt Foundation,\nthe Leverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation, and the Alfred P.\nSloan Foundation. LIGO DCC No. LIGO-P0900026.\n\nPublished - Abbott2009p6080Phys_Rev_D.pdf
", "abstract": "We report on a matched-filter search for gravitational wave bursts from cosmic string cusps using LIGO data from the fourth science run (S4) which took place in February and March 2005. No gravitational waves were detected in 14.9 days of data from times when all three LIGO detectors were operating. We interpret the result in terms of a frequentist upper limit on the rate of gravitational wave bursts and use the limits on the rate to constrain the parameter space (string tension, reconnection probability, and loop sizes) of cosmic string models. Many grand unified theory-scale models (with string tension G\u00b5/c^2[approximate]10^(-6)) can be ruled out at 90% confidence for reconnection probabilities p<=10^(-3) if loop sizes are set by gravitational back reaction.", "date": "2009-09-23", "date_type": "published", "publication": "Physical Review D", "volume": "80", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 062002", "id_number": "CaltechAUTHORS:20091021-153057198", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20091021-153057198", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Astronomy Research Council (UK)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "NASA" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Alexander von Humboldt Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P0900026", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "Space-Radiation-Laboratory" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.80.062002", "primary_object": { "basename": "Abbott2009p6080Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/q2zx5-xyq27/files/Abbott2009p6080Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2009", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/bmkej-wqj83", "eprint_id": 16469, "eprint_status": "archive", "datestamp": "2023-08-19 00:05:01", "lastmod": "2023-10-19 22:16:46", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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E." }, "orcid": "0000-0002-2544-1596" }, { "id": "zur-M\u00fchlen-H", "name": { "family": "zur-M\u00fchlen", "given": "H." } }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2009 The American Physical Society. \n\nReceived 22 June 2009; published 9 September 2009. \n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory and the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nCouncil of Scientific and Industrial Research of India,\nthe Istituto Nazionale di Fisica Nucleare of Italy, the\nSpanish Ministerio de Educaci\u03ccn y Ciencia, the\nConselleria d'Economia, Hisenda i Innovaci\u03cc of the\nGovern de les Illes Balears, the Scottish Funding\nCouncil, the Scottish Universities Physics Alliance, The\nNational Aeronautics and Space Administration, the\nCarnegie Trust, the Leverhulme Trust, the David and\nLucile Packard Foundation, the Research Corporation,\nand the Alfred P. Sloan Foundation. This paper was assigned\nLIGO document number LIGO-P080093.\n\nPublished - Abbott2009p6085Phys_Rev_D.pdf
", "abstract": "According to general relativity a perturbed black hole will settle to a stationary configuration by the\nemission of gravitational radiation. Such a perturbation will occur, for example, in the coalescence of a\nblack hole binary, following their inspiral and subsequent merger. At late times the waveform is a\nsuperposition of quasinormal modes, which we refer to as the ringdown. The dominant mode is expected\nto be the fundamental mode, l = m = 2. Since this is a well-known waveform, matched filtering can be\nimplemented to search for this signal using LIGO data. We present a search for gravitational waves from\nblack hole ringdowns in the fourth LIGO science run S4, during which LIGO was sensitive to the\ndominant mode of perturbed black holes with masses in the range of 10M_\u2609 to 500M_\u2609, the regime of\nintermediate-mass black holes, to distances up to 300 Mpc. We present a search for gravitational waves\nfrom black hole ringdowns using data from S4. No gravitational wave candidates were found; we place a\n90%-confidence upper limit on the rate of ringdowns from black holes with mass between 85M_\u2609 and\n390M_\u2609 in the local universe, assuming a uniform distribution of sources, of 3:2 X 10^(-5) yr^(-1) Mpc^(-3)=\n1:6 X 10^(-3) yr^(-1)L_10-^1 L_(10) ; where L_(10) is 10^(10) times the solar blue-light luminosity.", "date": "2009-09-15", "date_type": "published", "publication": "Physical Review D", "volume": "80", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 062001", "id_number": "CaltechAUTHORS:20091023-111958820", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20091023-111958820", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia, Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P080093", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.80.062001", "primary_object": { "basename": "Abbott2009p6085Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/bmkej-wqj83/files/Abbott2009p6085Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2009", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/4t5by-vnt12", "eprint_id": 15523, "eprint_status": "archive", "datestamp": "2023-08-21 22:07:10", "lastmod": "2023-10-19 14:32:00", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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E." }, "orcid": "0000-0002-2544-1596" }, { "id": "zur-M\u00fchlen-H", "name": { "family": "zur M\u00fchlen", "given": "H." } }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Stacked Search for Gravitational Waves from the 2006 SGR 1900+14 Storm", "ispublished": "pub", "full_text_status": "public", "keywords": "gamma rays: bursts; gravitational waves; pulsars: individual (SGR 1900+14); stars: neutron", "note": "\u00a9 2009 American Astronomical Society. \n\nPrint publication: Issue 2 (2009 August 20); received 2009 May 19; accepted for publication 2009 July 17; published 2009 July 30. \n\nThe authors are grateful to the Swift team for the SGR\n1900+14 storm data. The authors gratefully acknowledge the\nsupport of the United States National Science Foundation\nfor the construction and operation of the LIGO Laboratory\nand the Science and Technology Facilities Council of the\nUnited Kingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction and\noperation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u00b4on y Ciencia, the Conselleria d'Economia Hisenda i Innovaci\u00b4o of the Govern de les Illes Balears, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This Letter is LIGO-P0900024.\n\nPublished - Abbott2009p5729Astrophys_J_Lett.pdf
", "abstract": "We present the results of a LIGO search for short-duration gravitational waves (GWs) associated with the 2006 March 29 SGR 1900+14 storm. A new search method is used, \"stacking\" the GW data around the times of individual soft-gamma bursts in the storm to enhance sensitivity for models in which multiple bursts are accompanied by GW emission. We assume that variation in the time difference between burst electromagnetic emission and potential burst GW emission is small relative to the GW signal duration, and we time-align GW excess power time-frequency tilings containing individual burst triggers to their corresponding electromagnetic emissions. We use two GW emission models in our search: a fluence-weighted model and a flat (unweighted) model for the most electromagnetically energetic bursts. We find no evidence of GWs associated with either model. Model-dependent GW strain, isotropic GW emission energy E_(GW), and \u03b3 \u2261 E_(GW)/E_(EM) upper limits are estimated using a variety of assumed waveforms. The stacking method allows us to set the most stringent model-dependent limits on transient GW strain published to date. We find E_(GW) upper limit estimates (at a nominal distance of 10 kpc) of between 2 \u00d7 10^(45) erg and 6 \u00d7 10^(50) erg depending on the waveform type. These limits are an order of magnitude lower than upper limits published previously for this storm and overlap with the range of electromagnetic energies emitted in soft gamma repeater (SGR) giant flares.", "date": "2009-08-20", "date_type": "published", "publication": "Astrophysical Journal Letters", "volume": "701", "number": "2", "publisher": "American Astronomical Society", "pagerange": "L68-L74", "id_number": "CaltechAUTHORS:20090901-112329874", "issn": "2041-8205", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20090901-112329874", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "doi": "10.1088/0004-637X/701/2/L68", "primary_object": { "basename": "Abbott2009p5729Astrophys_J_Lett.pdf", "url": "https://authors.library.caltech.edu/records/4t5by-vnt12/files/Abbott2009p5729Astrophys_J_Lett.pdf" }, "resource_type": "article", "pub_year": "2009", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/swghf-c6b78", "eprint_id": 16411, "eprint_status": "archive", "datestamp": "2023-08-20 02:34:50", "lastmod": "2023-10-19 22:12:25", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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E." }, "orcid": "0000-0002-2544-1596" }, { "id": "zur-M\u00fchlen-H", "name": { "family": "zur-M\u00fchlen", "given": "H." } }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Einstein@Home search for periodic gravitational waves in early S5 LIGO data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2009 The American Physical Society. \n\nReceived 29 May 2009; published 11 August 2009. \n\nThe authors thank the tens of thousands of volunteers\nwho have supported the Einstein@Home project by donating\ntheir computer time and expertise for this analysis.\nWithout their contributions, this work would not have\nbeen possible. The authors gratefully acknowledge the\nsupport of the United States National Science Foundation\nfor the construction and operation of the LIGO Laboratory\nand the Science and Technology Facilities Council of the\nUnited Kingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nCouncil of Scientific and Industrial Research of India,\nthe Istituto Nazionale di Fisica Nucleare of Italy, the\nSpanish Ministerio de Educaci\u03ccn y Ciencia, the\nConselleria d'Economia, Hisenda i Innovaci\u03cc of the\nGovern de les Illes Balears, the Royal Society, the\nScottish Funding Council, the Scottish Universities\nPhysics Alliance, The National Aeronautics and Space\nAdministration, the Carnegie Trust, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan\nFoundation. This document has been assigned LIGO\nLaboratory document number LIGO-P0900032-v5.\n\nPublished - Abbott2009p5957Phys_Rev_D.pdf
", "abstract": "This paper reports on an all-sky search for periodic gravitational waves from sources such as deformed\nisolated rapidly spinning neutron stars. The analysis uses 840 hours of data from 66 days of the fifth LIGO\nscience run (S5). The data were searched for quasimonochromatic waves with frequencies f in the range\nfrom 50 to 1500 Hz, with a linear frequency drift _\u0192 (measured at the solar system barycenter) in the range\n-\u0192/T < \u0192_ < 0:1\u0192/T, for a minimum spin-down age T of 1000 years for signals below 400 Hz and\n8000 years above 400 Hz. The main computational work of the search was distributed over approximately\n100 000 computers volunteered by the general public. This large computing power allowed the use of a\nrelatively long coherent integration time of 30 hours while searching a large parameter space. This search\nextends Einstein@Home's previous search in LIGO S4 data to about 3 times better sensitivity. No\nstatistically significant signals were found. In the 125\u2013225 Hz band, more than 90% of sources with\ndimensionless gravitational-wave strain tensor amplitude greater than 3 X 10^(-24) would have been\ndetected.", "date": "2009-08-15", "date_type": "published", "publication": "Physical Review D", "volume": "80", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 042003", "id_number": "CaltechAUTHORS:20091020-142129445", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20091020-142129445", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia, Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "P0900032-v5", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.80.042003", "primary_object": { "basename": "Abbott2009p5957Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/swghf-c6b78/files/Abbott2009p5957Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2009", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/jrvvs-hc868", "eprint_id": 16210, "eprint_status": "archive", "datestamp": "2023-08-20 02:34:42", "lastmod": "2023-10-19 22:01:53", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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G." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Wooley-R", "name": { "family": "Wooley", "given": "R." } }, { "id": "Worden-J", "name": { "family": "Worden", "given": "J." } }, { "id": "Wu-W", "name": { "family": "Wu", "given": "W." } }, { "id": "Yakushin-I", "name": { "family": "Yakushin", "given": "I." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yan-Z", "name": { "family": "Yan", "given": "Z." } }, { "id": "Yoshida-S", "name": { "family": "Yoshida", "given": "S." } }, { "id": "Zanolin-M", "name": { "family": "Zanolin", "given": "M." } }, { "id": "Zhang-J", "name": { "family": "Zhang", "given": "J." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zhao-Chunnong", "name": { "family": "Zhao", "given": "C." }, "orcid": "0000-0001-5825-2401" }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "zur-M\u00fchlen-H", "name": { "family": "zur M\u00fchlen", "given": "H." } }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for gravitational waves from low mass compact binary coalescence in 186 days of LIGO's fifth science run", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2009 American Physical Society. \n\nReceived 18 June 2009; published 25 August 2009. \n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory and the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nCouncil of Scientific and Industrial Research of India,\nthe Istituto Nazionale di Fisica Nucleare of Italy, the\nSpanish Ministerio de Educacio\u00b4n y Ciencia, the\nConselleria d'Economia, Hisenda i Innovacio\u00b4 of the\nGovern de les Illes Balears, the Royal Society, the\nScottish Funding Council, the Scottish Universities\nPhysics Alliance, The National Aeronautics and Space\nAdministration, the Carnegie Trust, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - Abbott2009p5956Phys_Rev_D.pdf
", "abstract": "We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M_\u2609, using LIGO observations between November 14, 2006 and May 18, 2007. No gravitational-wave signals were detected. We report upper limits on the rate of compact binary coalescence as a function of total mass. The LIGO cumulative 90%-confidence rate upper limits of the binary coalescence of neutron stars, black holes and black hole-neutron star systems are 1.4 \u00d7 10^(-2), 7.3 \u00d7 10(-4) and 3.6 \u00d7 10(-3) yr(-1) L_10^(-1), respectively, where L_(10_ is 10^(10) times the blue solar luminosity", "date": "2009-08-15", "date_type": "published", "publication": "Physical Review D", "volume": "80", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 047101", "id_number": "CaltechAUTHORS:20091007-094829151", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20091007-094829151", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia, Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.80.047101", "primary_object": { "basename": "Abbott2009p5956Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/jrvvs-hc868/files/Abbott2009p5956Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2009", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/nvpc9-nk763", "eprint_id": 16208, "eprint_status": "archive", "datestamp": "2023-08-20 02:04:55", "lastmod": "2023-10-19 22:01:44", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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L." } }, { "id": "Weidner-A", "name": { "family": "Weidner", "given": "A." } }, { "id": "Weinert-M", "name": { "family": "Weinert", "given": "M." } }, { "id": "Weiss-R", "name": { "family": "Weiss", "given": "R." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Wen-S", "name": { "family": "Wen", "given": "S." } }, { "id": "Wette-K", "name": { "family": "Wette", "given": "K." } }, { "id": "Whelan-J-T", "name": { "family": "Whelan", "given": "J. T." } }, { "id": "Whitcomb-Stanley-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Whiting-B-F", "name": { "family": "Whiting", "given": "B. F." }, "orcid": "0000-0002-8501-8669" }, { "id": "Wilkinson-C", "name": { "family": "Wilkinson", "given": "C." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Williams-H-R", "name": { "family": "Williams", "given": "H. R." } }, { "id": "Williams-L", "name": { "family": "Williams", "given": "L." } }, { "id": "Willke-B", "name": { "family": "Willke", "given": "B." } }, { "id": "Wilmut-I", "name": { "family": "Wilmut", "given": "I." } }, { "id": "Winkelmann-L", "name": { "family": "Winkelmann", "given": "L." } }, { "id": "Winkler-W", "name": { "family": "Winkler", "given": "W." } }, { "id": "Wipf-Christopher-C", "name": { "family": "Wipf", "given": "C. C." } }, { "id": "Wiseman-A-G", "name": { "family": "Wiseman", "given": "A. G." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Wooley-R", "name": { "family": "Wooley", "given": "R." } }, { "id": "Worden-John-R", "name": { "family": "Worden", "given": "J." }, "orcid": "0000-0003-0257-9549" }, { "id": "Wu-W", "name": { "family": "Wu", "given": "W." } }, { "id": "Yakushin-I", "name": { "family": "Yakushin", "given": "I." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yan-Z", "name": { "family": "Yan", "given": "Z." } }, { "id": "Yoshida-S", "name": { "family": "Yoshida", "given": "S." } }, { "id": "Zanolin-M", "name": { "family": "Zanolin", "given": "M." } }, { "id": "Zhang-J", "name": { "family": "Zhang", "given": "J." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zhao-Chunnong", "name": { "family": "Zhao", "given": "C." }, "orcid": "0000-0001-5825-2401" }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-Michael-E", "name": { "family": "Zucker", "given": "M. E." }, "orcid": "0000-0002-2544-1596" }, { "id": "zur-M\u00fchlen-H", "name": { "family": "zur-M\u00fchlen", "given": "H." } }, { "id": "Zweizig-John", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for gravitational waves from low mass binary coalescences in the first year of LIGO's S5 data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a92009 The American Physical Society. \n\nReceived 11 February 2009; published 5 June 2009. \n\nThe authors thank Marie Anne Bizouard for her time and\nhelp in reviewing the accuracy of this research. The authors\ngratefully acknowledge the support of the U.S. National\nScience Foundation for the construction and operation of\nthe LIGO Laboratory, and the Science and Technology\nFacilities Council of the United Kingdom, the Max-\nPlanck-Society, and the State of Niedersachsen/Germany\nfor support of the construction and operation of the\nGEO600 detector. The authors also gratefully acknowledge\nthe support of the research by these agencies and by\nthe Australian Research Council, the Council of Scientific\nand Industrial Research of India, the Istituto Nazionale di\nFisica Nucleare of Italy, the Spanish Ministerio de\nEducaci\u03ccn y Ciencia, the Conselleria d'Economia,\nHisenda i Innovaci\u03cc of the Govern de les Illes Balears,\nthe Royal Society, the Scottish Funding Council, the\nScottish Universities Physics Alliance, the National\nAeronautics and Space Administration, the Carnegie\nTrust, the Leverhulme Trust, the David and Lucile\nPackard Foundation, the Research Corporation, and the\nAlfred P. Sloan Foundation.\n\nPublished - Abbott2009p5063Phys_Rev_D.pdf
", "abstract": "We have searched for gravitational waves from coalescing low mass compact binary systems with a total mass between 2M_([sun]) and 35Mz-([sun]) and a minimum component mass of 1M_([sun]) using data from the first year of the fifth science run of the three LIGO detectors, operating at design sensitivity. Depending on the mass, we are sensitive to coalescences as far as 150 Mpc from the Earth. No gravitational-wave signals were observed above the expected background. Assuming a population of compact binary objects with a Gaussian mass distribution representing binary neutron star systems, black hole\u2013neutron star binary systems, and binary black hole systems, we calculate the 90% confidence upper limit on the rate of coalescences to be 3.9\u00d710^(-2) yr^(-1)L_(10)^(-1), 1.1\u00d710^(-2) yr^(-1)L_(10)^(-1), and 2.5\u00d710^(-3)yr^(-1)L_(10)^(-1), respectively, where L_(10) is 10^(10) times the blue solar luminosity. We also set improved upper limits on the rate of compact binary coalescences per unit blue-light luminosity, as a function of mass.", "date": "2009-06-15", "date_type": "published", "publication": "Physical Review D", "volume": "79", "number": "12", "publisher": "American Physical Society", "pagerange": "Art. 122001", "id_number": "CaltechAUTHORS:20091007-073406265", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20091007-073406265", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" }, { "agency": "Royal Society" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.79.122001", "primary_object": { "basename": "Abbott2009p5063Phys_Rev_D.pdf", "url": "https://authors.library.caltech.edu/records/nvpc9-nk763/files/Abbott2009p5063Phys_Rev_D.pdf" }, "resource_type": "article", "pub_year": "2009", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/6yxvs-xrz96", "eprint_id": 13439, "eprint_status": "archive", "datestamp": "2023-08-22 12:58:48", "lastmod": "2023-10-17 23:53:49", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Babak-S", "name": { "family": "Babak", "given": "Stanislav" } }, { "id": "Baker-J-G", "name": { "family": "Baker", "given": "John G." } }, { "id": "Benacquista-M-J", "name": { "family": "Benacquista", "given": "Matthew J." } }, { "id": "Cornish-N-J", "name": { "family": "Cornish", "given": "Neil J." } }, { "id": "Crowder-J", "name": { "family": "Crowder", "given": "Jeff" } }, { "id": "Larson-S-L", "name": { "family": "Larson", "given": "Shane L." } }, { "id": "Plagnol-E", "name": { "family": "Plagnol", "given": "Eric" } }, { "id": "Porter-E-K", "name": { "family": "Porter", "given": "Edward K." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" }, { "id": "Vecchio-A", "name": { "family": "Vecchio", "given": "Alberto" }, "orcid": "0000-0002-6254-1617" }, { "id": "Arnaud-K", "name": { "family": "Arnaud", "given": "Keith" } }, { "id": "Barack-L", "name": { "family": "Barack", "given": "Leor" } }, { "id": "Blaut-A", "name": { "family": "Blaut", "given": "Arkadiusz" } }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "Curt" } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "Stephen" } }, { "id": "Gair-J-R", "name": { "family": "Gair", "given": "Jonathan" } }, { "id": "Gong-X", "name": { "family": "Gong", "given": "Xuefei" } }, { "id": "Harry-I", "name": { "family": "Harry", "given": "Ian" } }, { "id": "Khurana-D", "name": { "family": "Khurana", "given": "Deepak" } }, { "id": "Krolak-A", "name": { "family": "Krolak", "given": "Andrzej" } }, { "id": "Mandel-I", "name": { "family": "Mandel", "given": "Ilya" }, "orcid": "0000-0002-6134-8946" }, { "id": "Prix-R", "name": { "family": "Prix", "given": "Reinhard" } }, { "id": "Sathyaprakash-B-S", "name": { "family": "Sathyaprakash", "given": "B. S." } }, { "id": "Savov-P", "name": { "family": "Savov", "given": "Pavlin" } }, { "id": "Shang-Yu", "name": { "family": "Shang", "given": "Yu" } }, { "id": "Trias-M", "name": { "family": "Trias", "given": "Miquel" } }, { "id": "Veitch-J", "name": { "family": "Veitch", "given": "John" } }, { "id": "Wang-Yan", "name": { "family": "Wang", "given": "Yan" } }, { "id": "Wen-Linqing", "name": { "family": "Wen", "given": "Linqing" } }, { "id": "Whelan-J-T", "name": { "family": "Whelan", "given": "John T." } } ] }, "title": "The Mock LISA data challenges: from challenge 1B to challenge 3", "ispublished": "pub", "full_text_status": "restricted", "keywords": "POPULATION; BINARIES.", "note": "\u00a9 2008. Received 21 April 2008, in final form 11 June 2008.\nPublished 2 September 2008.\nSB and EP were supported by the Deutsches Zentrum f\u00fcr Luft-und Raumfahrt; LW's work by the Alexander von Humboldt Foundation's Sofja Kovalevskaja Programme funded by the\nGerman Federal Ministry of Education and Research. JG thanks the Royal Society for support and the Albert Einstein Institute for hospitality and support while part of this work was being completed. SF was supported by the Royal Society, BSS and IH by the UK Science and Technology Facilities Council. MV was supported by the LISA Mission Science Office andby JPL's HRDF. CC's, JC's and MV's work was carried out at the Jet Propulsion Laboratory,\nCalifornia Institute of Technology, under contract with the National Aeronautics and Space Administration. MTacknowledges support from the Spanish Ministerio de Educacion y Ciencia Research projects FPA-2007-60220, CSD207-00042 and the Govern de les Illes Balears,\nConselleria d'Economia, Hisenda i Innovaci\u03cc. IM was partially supported by NASA ATP grant NNX07AH22G to Northwestern University. PACS numbers: 04.80.Nn, 95.55.Ym", "abstract": "The Mock LISA Data Challenges are a programme to demonstrate and encourage the development of LISA data-analysis capabilities, tools and techniques. At the time of this workshop, three rounds of challenges had been completed, and the next was about to start. In this paper we provide a critical analysis of the entries to the latest completed round, Challenge 1B. The entries confirm the consolidation of a range of data-analysis techniques for\ngalactic and massive-black-hole binaries, and they include the first convincing examples of detection and parameter estimation of extreme-mass-ratio inspiral sources. In this paper we also introduce the next round, Challenge 3. Its data sets feature more realistic waveform models (e.g., galactic binaries may now chirp, and massive-black-hole binaries may precess due to spin interactions), as well as new source classes (bursts from cosmic strings, isotropic stochastic backgrounds) and more complicated nonsymmetric instrument noise.", "date": "2008-09-02", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "25", "number": "18", "publisher": "IOP", "pagerange": "184026", "id_number": "CaltechAUTHORS:BABcqg08b", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:BABcqg08b", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "Spanish Ministerio de Educacion y Ciencia", "grant_number": "FPA-2007-60220" }, { "agency": "Spanish Ministerio de Educacion y Ciencia", "grant_number": "CSD207-00042" }, { "agency": "NASA", "grant_number": "NNX07AH22G" }, { "agency": "Govern de les Illes Balears, Conselleria d'Economia, Hisenda i Innovaci\u03cc" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/25/18/184026", "resource_type": "article", "pub_year": "2008", "author_list": "Babak, Stanislav; Baker, John G.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/jg8jk-62537", "eprint_id": 45884, "eprint_status": "archive", "datestamp": "2023-08-19 23:27:14", "lastmod": "2023-10-26 18:31:11", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L-M", "name": { "family": "Goggin", "given": "L. M." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Messaritaki-E", "name": { "family": "Messaritaki", "given": "E." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Search of S3 LIGO data for gravitational wave signals from spinning black hole and neutron star binary inspirals", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2008 The American Physical Society.\n\nReceived 29 January 2008; published 6 August 2008.\n\nThe authors gratefully acknowledge the support of the\nU.S. National Science Foundation for the construction and\noperation of the LIGO Laboratory, and the Science and\nTechnology Facilities Council of the United Kingdom, the\nMax-Planck-Society, and the State of Niedersachsen/\nGermany for support of the construction and operation of\nthe GEO600 detector. The authors also gratefully acknowledge\nthe support of the research by these agencies and by\nthe Australian Research Council, the Council of Scientific\nand Industrial Research of India, the Istituto Nazionale di\nFisica Nucleare of Italy, the Spanish Ministerio de\nEducaci\u00f3n y Ciencia, the Conselleria d'Economia,\nHisenda i Innovaci\u00f3 of the Govern de les Illes Balears,\nthe Scottish Funding Council, the Scottish Universities\nPhysics Alliance, the National Aeronautics and Space\nAdministration, the Carnegie Trust, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - PhysRevD.78.042002.pdf
Submitted - 0712.2050v3.pdf
", "abstract": "We report on the methods and results of the first dedicated search for gravitational waves emitted during the inspiral of compact binaries with spinning component bodies. We analyze 788 hours of data collected during the third science run (S3) of the LIGO detectors. We searched for binary systems using a detection template family specially designed to capture the effects of the spin-induced precession of the orbital plane. We present details of the techniques developed to enable this search for spin-modulated gravitational waves, highlighting the differences between this and other recent searches for binaries with nonspinning components. The template bank we employed was found to yield high matches with our spin-modulated target waveform for binaries with masses in the asymmetric range 1.0M\u2299", "date": "2008-08-06", "date_type": "published", "publication": "Physical Review D", "volume": "78", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 042002", "id_number": "CaltechAUTHORS:20140522-094029718", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140522-094029718", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/ Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "Conselleria d'Economia, Hisenda i Innovaci\u00f3 of the Govern de les Illes Balears" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.78.042002", "primary_object": { "basename": "0712.2050v3.pdf", "url": "https://authors.library.caltech.edu/records/jg8jk-62537/files/0712.2050v3.pdf" }, "related_objects": [ { "basename": "PhysRevD.78.042002.pdf", "url": "https://authors.library.caltech.edu/records/jg8jk-62537/files/PhysRevD.78.042002.pdf" } ], "resource_type": "article", "pub_year": "2008", "author_list": "Abbott, B.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/wd7gf-ydw24", "eprint_id": 13530, "eprint_status": "archive", "datestamp": "2023-08-22 11:57:43", "lastmod": "2023-10-17 23:58:12", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Babak-S", "name": { "family": "Babak", "given": "S." } }, { "id": "Baker-J-G", "name": { "family": "Baker", "given": "J. G." } }, { "id": "Benacquista-M-J", "name": { "family": "Benacquista", "given": "M. J." } }, { "id": "Cornish-N-J", "name": { "family": "Cornish", "given": "N. J." } }, { "id": "Crowder-J", "name": { "family": "Crowder", "given": "J." } }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Larson-S-L", "name": { "family": "Larson", "given": "S. L." } }, { "id": "Littenberg-T-B", "name": { "family": "Littenberg", "given": "T. B." } }, { "id": "Porter-E-K", "name": { "family": "Porter", "given": "E. K." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vecchio-A", "name": { "family": "Vecchio", "given": "A." }, "orcid": "0000-0002-6254-1617" }, { "id": "Auger-G", "name": { "family": "Auger", "given": "G." } }, { "id": "Barack-L", "name": { "family": "Barack", "given": "L." } }, { "id": "Blaut-A", "name": { "family": "Blaut", "given": "A." } }, { "id": "Bloomer-E", "name": { "family": "Bloomer", "given": "E." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Christensen-N", "name": { "family": "Christensen", "given": "N." } }, { "id": "Clark-J", "name": { "family": "Clark", "given": "J." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Gair-J-R", "name": { "family": "Gair", "given": "J. R." } }, { "id": "Halloin-H", "name": { "family": "Halloin", "given": "H." } }, { "id": "Hendry-M", "name": { "family": "Hendry", "given": "M." } }, { "id": "Jimenez-A", "name": { "family": "Jimenez", "given": "A." } }, { "id": "Krolak-A", "name": { "family": "Krolak", "given": "A." } }, { "id": "Mandel-I", "name": { "family": "Mandel", "given": "I." }, "orcid": "0000-0002-6134-8946" }, { "id": "Messenger-C", "name": { "family": "Messenger", "given": "C." } }, { "id": "Meyer-R", "name": { "family": "Meyer", "given": "R." } }, { "id": "Mohanty-S", "name": { "family": "Mohanty", "given": "S." } }, { "id": "Nayak-R", "name": { "family": "Nayak", "given": "R." } }, { "id": "Petiteau-A", "name": { "family": "Petiteau", "given": "A." } }, { "id": "Pitkin-M", "name": { "family": "Pitkin", "given": "M." } }, { "id": "Plagnol-E", "name": { "family": "Plagnol", "given": "E." } }, { "id": "Prix-R", "name": { "family": "Prix", "given": "R." } }, { "id": "Robinson-E-L", "name": { "family": "Robinson", "given": "E. L." } }, { "id": "Roever-C", "name": { "family": "Roever", "given": "C." } }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Stroeer-A", "name": { "family": "Stroeer", "given": "A." } }, { "id": "Toher-J", "name": { "family": "Toher", "given": "J." } }, { "id": "Veitch-J", "name": { "family": "Veitch", "given": "J." } }, { "id": "Vinet-J-Y", "name": { "family": "Vinet", "given": "J. Y." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whelan-J-T", "name": { "family": "Whelan", "given": "J. T." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } } ] }, "title": "Report on the second Mock LISA data challenge", "ispublished": "pub", "full_text_status": "restricted", "keywords": "BLACK-HOLE BINARIES; SEARCH.", "note": "\u00a9 2008 IOP Publishing Ltd. Received 11 November 2007.\nPublished 15 May 2008.\nSB, EKP and JTW acknowledge support from the German Aerospace Center (DLR) and the Max-Planck Society. MB: from NASA grant NNG04GD52G and the NASA Center for GW Astronomy at the University of Texas, Brownsville (NAG5-13396). NC: NASA grants NNG05GI69G and NNX07AJ61G.MV: the LISAMission Science Office and by JPL'sHRDF. DB and SF: NSF grant PHY-0601459 and the LIGO Laboratory JG: St Catharine's College,\nCambridge. IM: the Brinson Foundation, NASA grant NNG04GK98G and NSF grant PHY-0601459. RP: the Max-Planck Society. LW: the Alexander von Humboldt Foundation's Sofja\nKovalevskaja program, funded by the German Federal Ministry of Education and Research. JC's, CC's and MV's work was carried out at the Jet Propulsion laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.\nPACS numbers: 04.80.Nn, 95.55.Ym", "abstract": "The Mock LISA data challenges are a program to demonstrate LISA data-analysis capabilities and to encourage their development. Each round of challenges consists of several data sets containing simulated instrument noise and gravitational waves from sources of undisclosed parameters. Participants are asked to analyze the data sets and report the maximum information about the source parameters. The challenges are being released in rounds of increasing complexity and realism: here we present the results of Challenge 2, issued in Jan 2007, which successfully demonstrated the recovery of signals from nonspinning supermassive-black-hole binaries with optimal SNRs between ~ 10 and 2000, from ~20 000 overlapping galactic white-dwarf binaries (among a realistically distributed population of 26 million), and from the extreme-mass-ratio inspirals of compact objects into central galactic black holes with optimal SNRs ~ 100.", "date": "2008-06-07", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "25", "number": "11", "publisher": "IOP", "pagerange": "114037", "id_number": "CaltechAUTHORS:BABcqg08a", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:BABcqg08a", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NASA", "grant_number": "NNG04GD52G" }, { "agency": "NASA", "grant_number": "NNG05GI69G" }, { "agency": "NASA", "grant_number": "NNX07AJ61G" }, { "agency": "NASA", "grant_number": "NAG5-13396" }, { "agency": "NASA", "grant_number": "NNG04GK98G" }, { "agency": "NSF", "grant_number": "PHY-0601459" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/25/11/114037", "resource_type": "article", "pub_year": "2008", "author_list": "Babak, S.; Baker, J. G.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/gn2st-2fd38", "eprint_id": 9736, "eprint_status": "archive", "datestamp": "2023-08-22 11:22:55", "lastmod": "2023-10-16 22:27:29", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" }, { "id": "Crowder-J", "name": { "family": "Crowder", "given": "Jeff" } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "Massimo" }, "orcid": "0000-0002-8107-5148" } ] }, "title": "Sensitivity and parameter-estimation precision for alternate LISA configurations", "ispublished": "pub", "full_text_status": "public", "note": "Copyright \u00a9 Institute of Physics and IOP Publishing Limited 2008. \n\nReceived 24 October 2007, in final form 4 February 2008. Published 4 March 2008. Print publication: Issue 6 (21 March 2008). \n\nThe authors are grateful to John Armstrong, Frank Estabrook, Tom Prince, Jan Harms, and to the anonymous referees for useful interactions. This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. MV was supported by LISA Mission Science Office and by JPL's Human Resources Development Fund. MT was supported under research task 05-BEFS05-0014. The supercomputers used in this investigation were provided by funding from the JPL Office of the Chief Information Officer.", "abstract": "We describe a simple framework to assess the LISA scientific performance (more specifically, its sensitivity and expected parameter-estimation precision for prescribed gravitational-wave signals) under the assumption of failure of one or two inter-spacecraft laser measurements (links) and of one to four intra-spacecraft laser measurements. We apply the framework to the simple case of measuring the LISA sensitivity to monochromatic circular binaries, and the LISA parameter-estimation precision for the gravitational-wave polarization angle of these systems. Compared to the six-link baseline configuration, the five-link case is characterized by a small loss in signal-to-noise ratio (SNR) in the high-frequency section of the LISA band; the four-link case shows a reduction by a factor of sqrt{2} at low frequencies, and by up to ~2 at high frequencies. The uncertainty in the estimate of polarization, as computed in the Fisher-matrix formalism, also worsens when moving from six to five, and then to four links: this can be explained by the reduced SNR available in those configurations (except for observations shorter than three months, where five and six links do better than four even with the same SNR). In addition, we prove (for generic signals) that the SNR and Fisher matrix are invariant with respect to the choice of a basis of TDI observables; rather, they depend only on which inter-spacecraft and intra-spacecraft measurements are available.", "date": "2008-03-21", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "25", "number": "6", "publisher": "IOP", "pagerange": "Art. No. 065005", "id_number": "CaltechAUTHORS:VALcqg08", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:VALcqg08", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/25/6/065005", "primary_object": { "basename": "VALcqg08.pdf", "url": "https://authors.library.caltech.edu/records/gn2st-2fd38/files/VALcqg08.pdf" }, "resource_type": "article", "pub_year": "2008", "author_list": "Vallisneri, Michele; Crowder, Jeff; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/3zjkw-r0g96", "eprint_id": 44559, "eprint_status": "archive", "datestamp": "2023-08-19 22:21:26", "lastmod": "2023-10-26 14:47:03", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "De-Salvo-R", "name": { "family": "De Salvo", "given": "R." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L-M", "name": { "family": "Goggin", "given": "L." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Messaritaki-E", "name": { "family": "Messaritaki", "given": "E." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Nocera-F", "name": { "family": "Nocera", "given": "F." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sanders-G-H", "name": { "family": "Sanders", "given": "G. H." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Tarallo-M", "name": { "family": "Tarallo", "given": "M." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Search for gravitational waves from binary inspirals in S3 and S4 LIGO data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2008 The American Physical Society. Received 26 April 2007; published 7 March 2008. The authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory and the\nScience and Technology Facilities Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nCouncil of Scientific and Industrial Research of India,\nthe Istituto Nazionale di Fisica Nucleare of Italy, the\nSpanish Ministerio de Educaci\u03ccn y Ciencia, the\nConselleria d'Economia, Hisenda i Innovaci\u03cc of the\nGovern de les Illes Balears, the Scottish Funding\nCouncil, the Scottish Universities Physics Alliance, The\nNational Aeronautics and Space Administration, the\nCarnegie Trust, the Leverhulme Trust, the David and\nLucile Packard Foundation, the Research Corporation,\nand the Alfred P. Sloan Foundation.\n\nPublished - PhysRevD.77.062002.pdf
Submitted - 0704.3368v4.pdf
", "abstract": "We report on a search for gravitational waves from the coalescence of compact binaries during the third and fourth LIGO science runs. The search focused on gravitational waves generated during the inspiral phase of the binary evolution. In our analysis, we considered three categories of compact binary systems, ordered by mass: (i) primordial black hole binaries with masses in the range 0.35M_\u2299", "date": "2008-03-07", "date_type": "published", "publication": "Physical Review D", "volume": "77", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 062002", "id_number": "CaltechAUTHORS:20140401-081124003", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140401-081124003", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (STFC)" }, { "agency": "Max-Planck-Society" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Istituto Nazionale di Fisica Nucleare (INFN)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Conselleria d'Economia, Hisenda i Innovaci\u03cc of the Govern de les Illes Balears" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.77.062002", "primary_object": { "basename": "0704.3368v4.pdf", "url": "https://authors.library.caltech.edu/records/3zjkw-r0g96/files/0704.3368v4.pdf" }, "related_objects": [ { "basename": "PhysRevD.77.062002.pdf", "url": "https://authors.library.caltech.edu/records/3zjkw-r0g96/files/PhysRevD.77.062002.pdf" } ], "resource_type": "article", "pub_year": "2008", "author_list": "Abbott, B.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/7htce-4aw75", "eprint_id": 45892, "eprint_status": "archive", "datestamp": "2023-08-19 22:16:07", "lastmod": "2023-10-26 18:31:28", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "M." }, "orcid": "0000-0002-8107-5148" }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Ding-H", "name": { "family": "Ding", "given": "H." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L", "name": { "family": "Goggin", "given": "L." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Logan-J", "name": { "family": "Logan", "given": "J." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Messaritaki-E", "name": { "family": "Messaritaki", "given": "E." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Nocera-F", "name": { "family": "Nocera", "given": "F." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sanders-G-H", "name": { "family": "Sanders", "given": "G. H." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Sylvestre-J", "name": { "family": "Sylvestre", "given": "J." } }, { "id": "Takamori-A", "name": { "family": "Takamori", "given": "A." } }, { "id": "Tarallo-M", "name": { "family": "Tarallo", "given": "M." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Search for gravitational waves associated with 39 gamma-ray bursts using data from the second, third, and fourth LIGO runs", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2008 The American Physical Society. Received 16 October 2007; published 17 March 2008. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacion y Ciencia, The\nNational Aeronautics and Space Administration, the John\nSimon Guggenheim Foundation, the Alexander von Humboldt Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory document number LIGOP060024-07-Z.\n\nPublished - PhysRevD.77.062004.pdf
Submitted - 0709.0766v2.pdf
", "abstract": "We present the results of a search for short-duration gravitational-wave bursts associated with 39 gamma-ray bursts (GRBs) detected by gamma-ray satellite experiments during LIGO's S2, S3, and S4 science runs. The search involves calculating the crosscorrelation between two interferometer data streams surrounding the GRB trigger time. We search for associated gravitational radiation from single GRBs, and also apply statistical tests to search for a gravitational-wave signature associated with the whole sample. For the sample examined, we find no evidence for the association of gravitational radiation with GRBs, either on a single-GRB basis or on a statistical basis. Simulating gravitational-wave bursts with sine-Gaussian waveforms, we set upper limits on the root-sum-square of the gravitational-wave strain amplitude of such waveforms at the times of the GRB triggers. We also demonstrate how a sample of several GRBs can be used collectively to set constraints on population models. The small number of GRBs and the significant change in sensitivity of the detectors over the three runs, however, limits the usefulness of a population study for the S2, S3, and S4 runs. Finally, we discuss prospects for the search sensitivity for the ongoing S5 run, and beyond for the next generation of detectors.", "date": "2008-03", "date_type": "published", "publication": "Physical Review D", "volume": "77", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 062004", "id_number": "CaltechAUTHORS:20140522-133958402", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140522-133958402", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "NASA" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Alexander von Humboldt Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "P060024-07-Z", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.77.062004", "primary_object": { "basename": "0709.0766v2.pdf", "url": "https://authors.library.caltech.edu/records/7htce-4aw75/files/0709.0766v2.pdf" }, "related_objects": [ { "basename": "PhysRevD.77.062004.pdf", "url": "https://authors.library.caltech.edu/records/7htce-4aw75/files/PhysRevD.77.062004.pdf" } ], "resource_type": "article", "pub_year": "2008", "author_list": "Abbott, B.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/t4faa-z5e25", "eprint_id": 9589, "eprint_status": "archive", "datestamp": "2023-08-22 11:08:41", "lastmod": "2023-10-16 22:22:26", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Use and abuse of the Fisher information matrix in the assessment of gravitational-wave parameter-estimation prospects", "ispublished": "pub", "full_text_status": "public", "note": "\u00a92008 The American Physical Society. \n\n(Received 15 March 2007; published 4 February 2008) \n\nI would like to thank Yanbei Chen, Curt Cutler, Yi Pan, and Michele Zanolin for useful discussions; for reviewing this manuscript, I am grateful to John Armstrong, Emanuele Berti, Steve Drasco, Frank Estabrook, Sam Finn, \u00c9anna Flanagan, and especially Alessandra Buonanno. My work was supported by the LISA Mission Science Office and by the Human Resources Development Fund at the Jet Propulsion Laboratory, California Institute of Technology, where it was performed under contract with the National Aeronautics and Space Administration.", "abstract": "The Fishermatrix formalism is used routinely in the literature on gravitational-wave detection to characterize the parameter-estimation performance of gravitational-wave measurements, given parametrized models of the waveforms, and assuming detector noise of known colored Gaussian distribution. Unfortunately, the Fisher matrix can be a poor predictor of the amount of information obtained from typical observations, especially for waveforms with several parameters and relatively low expected signal-to-noise ratios (SNR), or for waveforms depending weakly on one or more parameters, when their priors are not taken into proper consideration. In this paper I discuss these pitfalls; show how they occur, even for relatively strong signals, with a commonly used template family for binary-inspiral waveforms; and describe practical recipes to recognize them and cope with them. Specifically, I answer the following questions: (i) What is the significance of (quasi-)singular Fisher matrices, and how must we deal with them? (ii) When is it necessary to take into account prior probability distributions for the source parameters? (iii) When is the signal-to-noise ratio high enough to believe the Fisher-matrix result? In addition, I provide general expressions for the higher-order, beyond-Fisher-matrix terms in the 1/SNR expansions for the expected parameter accuracies.", "date": "2008-02-15", "date_type": "published", "publication": "Physical Review D", "volume": "77", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 042001", "id_number": "CaltechAUTHORS:VALprd08", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:VALprd08", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1103/PhysRevD.77.042001", "primary_object": { "basename": "VALprd08.pdf", "url": "https://authors.library.caltech.edu/records/t4faa-z5e25/files/VALprd08.pdf" }, "resource_type": "article", "pub_year": "2008", "author_list": "Vallisneri, Michele" }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/k0rrn-vf704", "eprint_id": 44546, "eprint_status": "archive", "datestamp": "2023-08-19 22:00:44", "lastmod": "2023-10-26 14:46:34", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L-M", "name": { "family": "Goggin", "given": "L. M." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-O", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Tarallo-M", "name": { "family": "Tarallo", "given": "M." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } } ] }, "title": "All-sky search for periodic gravitational waves in LIGO S4 data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2008 American Physical Society.\n\nReceived 11 September 2007; published 10 January 2008; publisher error corrected 29 February 2008.\n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction and operation of the LIGO Laboratory and the\nParticle Physics and Astronomy Research Council of the\nUnited Kingdom, the Max-Planck-Society and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nNatural Sciences and Engineering Research Council of\nCanada, the Council of Scientific and Industrial Research\nof India, the Department of Science and Technology of\nIndia, the Spanish Ministerio de Educacion y Ciencia, The\nNational Aeronautics and Space Administration, the John\nSimon Guggenheim Foundation, the Alexander von Humboldt Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory Document No. LIGO-P060010-05-Z.\n\nPublished - PhysRevD.77.022001.pdf
Submitted - 0708.3818v2.pdf
", "abstract": "We report on an all-sky search with the LIGO detectors for periodic gravitational waves in the frequency range 50\u20131000 Hz and with the frequency's time derivative in the range \u22121\u00d710^(\u22128)\u2009\u2009Hz\u2009s^(\u22121) to zero. Data from the fourth LIGO science run (S4) have been used in this search. Three different semicoherent methods of transforming and summing strain power from short Fourier transforms (SFTs) of the calibrated data have been used. The first, known as StackSlide, averages normalized power from each SFT. A \"weighted Hough\" scheme is also developed and used, which also allows for a multi-interferometer search. The third method, known as PowerFlux, is a variant of the StackSlide method in which the power is weighted before summing. In both the weighted Hough and PowerFlux methods, the weights are chosen according to the noise and detector antenna-pattern to maximize the signal-to-noise ratio. The respective advantages and disadvantages of these methods are discussed. Observing no evidence of periodic gravitational radiation, we report upper limits; we interpret these as limits on this radiation from isolated rotating neutron stars. The best population-based upper limit with 95% confidence on the gravitational-wave strain amplitude, found for simulated sources distributed isotropically across the sky and with isotropically distributed spin axes, is 4.28\u00d710^(\u221224) (near 140 Hz). Strict upper limits are also obtained for small patches on the sky for best-case and worst-case inclinations of the spin axes.", "date": "2008-01-10", "date_type": "published", "publication": "Physical Review D", "volume": "77", "number": "2", "publisher": "American Physical Society", "pagerange": "Art. No. 022001", "id_number": "CaltechAUTHORS:20140328-095155437", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140328-095155437", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "NASA" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Alexander von Humboldt Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P060010-05-Z", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.77.022001", "primary_object": { "basename": "0708.3818v2.pdf", "url": "https://authors.library.caltech.edu/records/k0rrn-vf704/files/0708.3818v2.pdf" }, "related_objects": [ { "basename": "PhysRevD.77.022001.pdf", "url": "https://authors.library.caltech.edu/records/k0rrn-vf704/files/PhysRevD.77.022001.pdf" } ], "resource_type": "article", "pub_year": "2008", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/rn13k-v1z76", "eprint_id": 43326, "eprint_status": "archive", "datestamp": "2023-08-19 21:30:13", "lastmod": "2023-10-25 23:28:10", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Brady-P-R", "name": { "family": "Brady", "given": "P. R." }, "orcid": "0000-0002-4611-9387" }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L-M", "name": { "family": "Goggin", "given": "L. M." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Messaritaki-E", "name": { "family": "Messaritaki", "given": "E." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Tarallo-M", "name": { "family": "Tarallo", "given": "M." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "M." }, "orcid": "0000-0002-8107-5148" }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } } ] }, "title": "Search for gravitational-wave bursts in LIGO data from the fourth science run", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2007 IOP Publishing Ltd. Received 3 May 2007, in final form 28 August 2007. Published 24 October 2007. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Science\nand Technology Facilities Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO 600 detector. The authors also gratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaci\u00f2n y Ciencia, the Conselleria d'Economia, Hisenda i Innovaci\u00f2 of the Govern de les Illes Balears, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P Sloan Foundation. This document has been assigned LIGO Laboratory document number LIGO-P060016-B-Z.\n\nSubmitted - 0704.0943v3.pdf
", "abstract": "The fourth science run of the LIGO and GEO 600 gravitational-wave detectors, carried out in early 2005, collected data with significantly lower noise than previous science runs. We report on a search for short-duration gravitational-wave bursts with arbitrary waveform in the 64\u20131600 Hz frequency range appearing in all three LIGO interferometers. Signal consistency tests, data quality cuts and auxiliary-channel vetoes are applied to reduce the rate of spurious triggers. No gravitational-wave signals are detected in 15.5 days of live observation time; we set a frequentist upper limit of 0.15 day^(\u22121) (at 90% confidence level) on the rate of bursts with large enough amplitudes to be detected reliably. The amplitude sensitivity of the search, characterized using Monte Carlo simulations, is several times better than that of previous searches. We also provide rough estimates of the distances at which representative supernova and binary black hole merger signals could be detected with 50% efficiency by this analysis.", "date": "2007-11-21", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "24", "number": "22", "publisher": "IOP", "pagerange": "5343-5369", "id_number": "CaltechAUTHORS:20140113-082240415", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140113-082240415", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Science and Technology Facilities Council (United Kingdom)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Scientific and Industrial Research of India" }, { "agency": "Istituto Nazionale di Fisica Nucleare, Italy" }, { "agency": "Spanish Ministerio de Educaci\u00f2n y Ciencia" }, { "agency": "Conselleria d'Economia Hisenda i Innovaci\u00f2 of the Govern de les Illes Balears" }, { "agency": "Scottish Funding Council" }, { "agency": "Scottish Universities Physics Alliance" }, { "agency": "NASA" }, { "agency": "Carnegie Trust" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P060016-B-Z", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1088/0264-9381/24/22/002", "primary_object": { "basename": "0704.0943v3.pdf", "url": "https://authors.library.caltech.edu/records/rn13k-v1z76/files/0704.0943v3.pdf" }, "resource_type": "article", "pub_year": "2007", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/a0tdm-twc23", "eprint_id": 44548, "eprint_status": "archive", "datestamp": "2023-08-19 21:19:36", "lastmod": "2023-10-26 14:46:40", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L-M", "name": { "family": "Goggin", "given": "L. M." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Messaritaki-E", "name": { "family": "Messaritaki", "given": "E." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Tarallo-M", "name": { "family": "Tarallo", "given": "M." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Upper limit map of a background of gravitational waves", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2007 American Physical Society. Received 31 January 2007. \nPublished 29 October 2007. Publisher error corrected 28 February 2008. The work described in this paper was part of the doctoral\nthesis of S.W. Ballmer at the Massachusetts Institute of\nTechnology [10]. Furthermore the authors gratefully acknowledge\nthe support of the U.S. National Science\nFoundation for the construction and operation of the\nLIGO Laboratory and the Particle Physics and\nAstronomy Research Council of the United Kingdom, the\nMax-Planck-Society, and the State of Niedersachsen,\nGermany, for support of the construction and operation\nof the GEO600 detector. The authors also gratefully acknowledge\nthe support of the research by these agencies\nand by the Australian Research Council, the Natural\nSciences and Engineering Research Council of Canada,\nthe Council of Scientific and Industrial Research of India,\nthe Department of Science and Technology of India, the\nSpanish Ministerio de Educacion y Ciencia, The National\nAeronautics and Space Administration, the John Simon\nGuggenheim Foundation, the Alexander von Humboldt\nFoundation, the Leverhulme Trust, the David and Lucile\nPackard Foundation, the Research Corporation, and the\nAlfred P. Sloan Foundation. This paper has been assigned\nthe LIGO document number LIGO-P060029-00-Z.\n\nPublished - PhysRevD.76.082003.pdf
Submitted - 0703234v1.pdf
", "abstract": "We searched for an anisotropic background of gravitational waves using data from the LIGO S4 science run and a method that is optimized for point sources. This is appropriate if, for example, the gravitational wave background is dominated by a small number of distinct astrophysical sources. No signal was seen. Upper limit maps were produced assuming two different power laws for the source strain power spectrum. For an f^(\u22123) power law and using the50 Hz to 1.8 kHz band the upper limits on the source strain power spectrum vary between 1.2\u00d710^(\u221248)\u2009\u2009Hz^(\u22121) (100\u2009\u2009Hz/f)^3 and 1.2\u00d710^(\u221247)\u2009\u2009Hz^(\u22121) (100\u2009\u2009Hz/f)^3, depending on the position in the sky. Similarly, in the case of constant strain power spectrum, the upper limits vary between 8.5\u00d710\u221249\u2009\u2009Hz\u22121 and 6.1\u00d710^(\u221248)\u2009\u2009Hz^(\u22121). As a side product a limit on an isotropic background of gravitational waves was also obtained. All limits are at the 90% confidence level. Finally, as an application, we focused on the direction of Sco-X1, the brightest low-mass x-ray binary. We compare the upper limit on strain amplitude obtained by this method to expectations based on the x-ray flux from Sco-X1.", "date": "2007-10-29", "date_type": "published", "publication": "Physical Review D", "volume": "76", "number": "8", "publisher": "American Physical Society", "pagerange": "art. No. 082003", "id_number": "CaltechAUTHORS:20140328-113831012", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140328-113831012", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "NASA" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Alexander von Humboldt Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Max-Planck-Gesellschaft" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P060029-00-Z", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.76.082003", "primary_object": { "basename": "0703234v1.pdf", "url": "https://authors.library.caltech.edu/records/a0tdm-twc23/files/0703234v1.pdf" }, "related_objects": [ { "basename": "PhysRevD.76.082003.pdf", "url": "https://authors.library.caltech.edu/records/a0tdm-twc23/files/PhysRevD.76.082003.pdf" } ], "resource_type": "article", "pub_year": "2007", "author_list": "Abbott, B.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/wr0hb-q8n03", "eprint_id": 44545, "eprint_status": "archive", "datestamp": "2023-08-19 21:09:14", "lastmod": "2023-10-26 14:46:31", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "M." }, "orcid": "0000-0002-8107-5148" }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Ding-H", "name": { "family": "Ding", "given": "H." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L-M", "name": { "family": "Goggin", "given": "L. M." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Logan-J", "name": { "family": "Logan", "given": "J." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Messaritaki-E", "name": { "family": "Messaritaki", "given": "E." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Nocera-F", "name": { "family": "Nocera", "given": "F." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sanders-G-H", "name": { "family": "Sanders", "given": "G. H." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Sylvestre-J", "name": { "family": "Sylvestre", "given": "J." } }, { "id": "Takamori-A", "name": { "family": "Takamori", "given": "A." } }, { "id": "Tarallo-M", "name": { "family": "Tarallo", "given": "M." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Searches for periodic gravitational waves from unknown isolated sources and Scorpius X-1: Results from the second LIGO science run", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2007 The American Physical Society. Received 12 June 2006. Revised 2 April 2007. Published 24 October 2007. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction\nand operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nNatural Sciences and Engineering Research Council of\nCanada, the Council of Scientific and Industrial Research\nof India, the Department of Science and Technology of\nIndia, the Spanish Ministerio de Educacion y Ciencia, The\nNational Aeronautics and Space Administration, the John\nSimon Guggenheim Foundation, the Alexander von\nHumboldt Foundation, the Leverhulme Trust, the David\nand Lucile Packard Foundation, the Research Corporation,\nand the Alfred P. Sloan Foundation. This document has\nbeen assigned LIGO Laboratory Document No. LIGO-P050008.\n\nPublished - PhysRevD.76.082001.pdf
Submitted - 0605028v2.pdf
", "abstract": "We carry out two searches for periodic gravitational waves using the most sensitive few hours of data from the second LIGO science run. Both searches exploit fully coherent matched filtering and cover wide areas of parameter space, an innovation over previous analyses which requires considerable algorithm development and computational power. The first search is targeted at isolated, previously unknown neutron stars, covers the entire sky in the frequency band 160\u2013728.8 Hz, and assumes a frequency derivative of less than 4\u00d710^(\u221210)\u2009\u2009Hz/s. The second search targets the accreting neutron star in the low-mass x-ray binary Scorpius X-1 and covers the frequency bands 464\u2013484 Hz and 604\u2013624 Hz as well as the two relevant binary orbit parameters. Because of the high computational cost of these searches we limit the analyses to the most sensitive 10 hours and 6 hours of data, respectively. Given the limited sensitivity and duration of the analyzed data set, we do not attempt deep follow-up studies. Rather we concentrate on demonstrating the data analysis method on a real data set and present our results as upper limits over large volumes of the parameter space. In order to achieve this, we look for coincidences in parameter space between the Livingston and Hanford 4-km interferometers. For isolated neutron stars our 95% confidence level upper limits on the gravitational wave strain amplitude range from 6.6\u00d710^(\u221223) to 1\u00d710^(\u221221) across the frequency band; for Scorpius X-1 they range from 1.7\u00d710^(\u221222) to 1.3\u00d710^(\u221221) across the two 20-Hz frequency bands. The upper limits presented in this paper are the first broadband wide parameter space upper limits on periodic gravitational waves from coherent search techniques. The methods developed here lay the foundations for upcoming hierarchical searches of more sensitive data which may detect astrophysical signals.", "date": "2007-10-24", "date_type": "published", "publication": "Physical Review D", "volume": "76", "number": "8", "publisher": "American Physical Society", "pagerange": "Art. No. 082001", "id_number": "CaltechAUTHORS:20140328-081826662", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140328-081826662", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "NASA" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Alexander von Humboldt Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P050008", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.76.082001", "primary_object": { "basename": "PhysRevD.76.082001.pdf", "url": "https://authors.library.caltech.edu/records/wr0hb-q8n03/files/PhysRevD.76.082001.pdf" }, "related_objects": [ { "basename": "0605028v2.pdf", "url": "https://authors.library.caltech.edu/records/wr0hb-q8n03/files/0605028v2.pdf" } ], "resource_type": "article", "pub_year": "2007", "author_list": "Abbott, B.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/ky4c2-0fy21", "eprint_id": 8892, "eprint_status": "archive", "datestamp": "2023-08-22 10:12:29", "lastmod": "2023-10-16 21:47:49", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Brown-D-A", "name": { "family": "Brown", "given": "Duncan A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Crowder-J", "name": { "family": "Crowder", "given": "Jeff" } }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "Curt" } }, { "id": "Mandel-I", "name": { "family": "Mandel", "given": "Ilya" }, "orcid": "0000-0002-6134-8946" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "A three-stage search for supermassive black-hole binaries in LISA data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 US Govt. \n\nReceived 19 April 2007, in final form 22 April 2007. Published 19 September 2007. Print publication: Issue 19 (7 October 2007). \n\nJC's, CC's and MV's work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract to the National Aeronautics and Space Administration. JC would like to thank the staff of the supercomputing facilities of the Jet Propulsion Laboratory, California Institute of Technology, where the MCMC stage of the searches described herein was carried out. IM would like to acknowledge the Brinson Foundation, NASA grant NNG04GK98G and NSF grant PHY-0601459 for financial support. MV is grateful for support from the Human Resources Development Fund program at JPL. DB acknowledges funding from NSF grant PHY-0601459 and the LIGO Laboratory. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation and operates under cooperative agreement PHY-0107417. This paper carries LIGO document number LIGO-P070018-00-Z. \n\nPROCEEDINGS OF THE 11TH GRAVITATIONAL WAVE DATA ANALYSIS WORKSHOP, POTSDAM, GERMANY, 18-21 DECEMBER 2006, Classical and Quantum Gravity, Volume 24, Number 19, 7 October 2007 http://www.iop.org/EJ/toc/0264-9381/24/19", "abstract": "Gravitational waves from the inspiral and coalescence of supermassive black-hole (SMBH) binaries with masses m1 ~ m2 ~ 10^6Modot are likely to be among the strongest sources for the Laser Interferometer Space Antenna (LISA). We describe a three-stage data-analysis pipeline designed to search for and measure the parameters of SMBH binaries in LISA data. The first stage uses a time\u2013frequency track-search method to search for inspiral signals and provide a coarse estimate of the black-hole masses m1, m2 and the coalescence time of the binary tc. The second stage uses a sequence of matched-filter template banks, seeded by the first stage, to improve the measurement accuracy of the masses and coalescence time. Finally, a Markov chain Monte Carlo search is used to estimate all nine physical parameters of the binary (masses, coalescence time, distance, initial phase, sky position and orientation). Using results from the second stage substantially shortens the Markov chain burn-in time and allows us to determine the number of SMBH-binary signals in the data before starting parameter estimation. We demonstrate our analysis pipeline using simulated data from the first Mock LISA Data Challenge. We discuss our plan for improving this pipeline and the challenges that will be faced in real LISA data analysis.", "date": "2007-10-07", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "24", "number": "19", "publisher": "IOP", "pagerange": "S595-S605", "id_number": "CaltechAUTHORS:BROcqg07", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:BROcqg07", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/24/19/S22", "primary_object": { "basename": "BROcqg07.pdf", "url": "https://authors.library.caltech.edu/records/ky4c2-0fy21/files/BROcqg07.pdf" }, "resource_type": "article", "pub_year": "2007", "author_list": "Brown, Duncan A.; Crowder, Jeff; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/ty5v1-d0q65", "eprint_id": 8893, "eprint_status": "archive", "datestamp": "2023-08-22 10:12:34", "lastmod": "2023-10-16 21:47:52", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Arnaud-K-A", "name": { "family": "Arnaud", "given": "K. A." } }, { "id": "Babak-S", "name": { "family": "Babak", "given": "S." } }, { "id": "Baker-J-G", "name": { "family": "Baker", "given": "J. G." } }, { "id": "Benacquista-M-J", "name": { "family": "Benacquista", "given": "M. J." } }, { "id": "Cornish-M-J", "name": { "family": "Cornish", "given": "M. J." } }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Finn-L-S", "name": { "family": "Finn", "given": "L. S." } }, { "id": "Larson-S-L", "name": { "family": "Larson", "given": "S. L." } }, { "id": "Littenberg-T", "name": { "family": "Littenberg", "given": "T." } }, { "id": "Porter-E-K", "name": { "family": "Porter", "given": "E. K." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vecchio-A", "name": { "family": "Vecchio", "given": "A." }, "orcid": "0000-0002-6254-1617" }, { "id": "Vinet-J-Y", "name": { "family": "Vinet", "given": "J-Y" } }, { "id": "Mock-LISA-Data-Challenge-Task-Force", "name": { "family": "Mock", "given": "LISA Data Challenge Task Force" } } ] }, "title": "An overview of the second round of the Mock LISA Data Challenges", "ispublished": "pub", "full_text_status": "public", "note": "Copyright \u00a9 Institute of Physics and IOP Publishing Limited 2007. \n\nReceived 4 April 2007. Published 19 September 2007. Print publication: Issue 19 (7 October 2007). \n\nMB acknowledges funding from NASA grant NNG04GD52G and support by the NASA Center for Gravitational Wave Astronomy at University of Texas at Brownsville (NAG5-13396). NC and TL acknowledge funding from NASA grant NNG05GI69G. The work of CC and MV was performed at the Jet Propulsion Laboratory, California Institute of Technology, where it was performed under contract with the National Aeronautics and Space Administration. MV was supported by the LISA Mission Science Office and by the Human Resources Development Fund at JPL. \n\nPROCEEDINGS OF THE 11TH GRAVITATIONAL WAVE DATA ANALYSIS WORKSHOP, POTSDAM, GERMANY, 18-21 DECEMBER 2006, Classical and Quantum Gravity, Volume 24, Number 19, 7 October 2007 http://www.iop.org/EJ/toc/0264-9381/24/19", "abstract": "The Mock Data Challenges (MLDCs) have the dual purpose of fostering the development of LISA data-analysis tools and capabilities and of demonstrating the technical readiness already achieved by the gravitational-wave community in distilling a rich science payoff from the LISA data. The first round of MLDCs has just been completed and the second-round data sets are being released shortly after this workshop. The second-round data sets contain radiation from an entire Galactic population of stellar-mass binary systems, from massive-black-hole binaries, and from extreme-mass-ratio inspirals. These data sets are designed to capture much of the complexity that is expected in the actual LISA data, and should provide a fairly realistic setting to test advanced data-analysis techniques, and in particular the global aspect of the analysis. Here we describe the second round of MLDCs and provide details about its implementation.", "date": "2007-10-07", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "24", "number": "19", "publisher": "IOP", "pagerange": "S551-S564", "id_number": "CaltechAUTHORS:ARNcqg07a", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ARNcqg07a", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/24/19/S18", "primary_object": { "basename": "ARNcqg07a.pdf", "url": "https://authors.library.caltech.edu/records/ty5v1-d0q65/files/ARNcqg07a.pdf" }, "resource_type": "article", "pub_year": "2007", "author_list": "Arnaud, K. A.; Babak, S.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/jwsj6-29g35", "eprint_id": 19666, "eprint_status": "archive", "datestamp": "2023-08-19 21:06:29", "lastmod": "2023-10-20 21:14:29", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Arnaud-K-A", "name": { "family": "Arnaud", "given": "K. A." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Mandel-I", "name": { "family": "Mandel", "given": "I." }, "orcid": "0000-0002-6134-8946" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Report on the first round of the Mock LISA Data Challenges", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2007 IOP Publishing.\n\nReceived 30 March 2007, in final form 2 April 2007.\nPublished 19 September 2007.\nMB acknowledges funding from NASA Grant NNG04GD52G. MB, SM and RN were\nsupported by the NASA Center for Gravitational Wave Astronomy at University of Texas\nat Brownsville (NAG5-13396). N Christensen acknowledges funding from NSF Grant PHY-\n0553422 and the Fulbright Scholar Program. N Cornish, J Crowder and EP acknowledge\nfunding from NASA Grant NNG05GI69G. J Crowder, CC and MV carried out this work at\nJPL, Caltech, under contract to NASA. MV is grateful for support from the Human Resources\nDevelopment Fund program at JPL. IM would like to thank the Brinson Foundation, NASA\nGrant NNG04GK98G and NSF Grant PHY-0601459. DB was supported by NSF Grant\nPHY-0601459 and the LIGO Laboratory. LIGO was constructed by the California Institute\nof Technology and Massachusetts Institute of Technology with funding from the National\nScience Foundation and operates under cooperative agreement PHY-0107417. The work of\nAK was supported in part by grant 1 P03B 029 27 from the Polish Ministry of Science and Information Technology. AK would like to acknowledge hospitality of Max Planck Institute\nfor Gravitational Physics in Potsdam, Germany, where part of his work was done. AV was\npartially supported by the Packard Foundation and the NSF.\n\nPublished - Arnaud2007p8885Classical_Quant_Grav.pdf
", "abstract": "The Mock LISA Data Challenges (MLDCs) have the dual purpose of fostering the development of LISA data analysis tools and capabilities, and demonstrating the technical readiness already achieved by the gravitational-wave community in distilling a rich science payoff from the LISA data output. The first round of MLDCs has just been completed: nine challenges consisting of data sets containing simulated gravitational-wave signals produced either by galactic binaries or massive black hole binaries embedded in simulated LISA instrumental noise were released in June 2006 with deadline for submission of results at the beginning of December 2006. Ten groups have participated in this first round of challenges. All of the challenges had at least one entry which successfully characterized the signal to better than 95% when assessed via a correlation with phasing ambiguities accounted for. Here, we describe the challenges, summarize the results and provide a first critical assessment of the entries.", "date": "2007-10-07", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "24", "number": "19", "publisher": "IOP", "pagerange": "S529-S539", "id_number": "CaltechAUTHORS:20100826-083744729", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100826-083744729", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NASA", "grant_number": "NNG04GD52G" }, { "agency": "University of Texas Brownsville NASA Center for Gravitational Wave Astronomy", "grant_number": "NAG5-13396" }, { "agency": "NSF", "grant_number": "PHY-0553422" }, { "agency": "Fulbright Scholar Program" }, { "agency": "NASA", "grant_number": "NNG05GI69G" }, { "agency": "JPL Human Resources Development Fund" }, { "agency": "Brinson Foundation" }, { "agency": "NASA", "grant_number": "NNG04GK98G" }, { "agency": "NSF", "grant_number": "PHY-0601459" }, { "agency": "NSF", "grant_number": "PHY-0601459" }, { "agency": "LIGO Laboratory" }, { "agency": "Polish Ministry of Science and Information Technology", "grant_number": "1 P03B 029 27" }, { "agency": "Packard Foundation" }, { "agency": "NSF" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/24/19/S16", "primary_object": { "basename": "Arnaud2007p8885Classical_Quant_Grav.pdf", "url": "https://authors.library.caltech.edu/records/jwsj6-29g35/files/Arnaud2007p8885Classical_Quant_Grav.pdf" }, "resource_type": "article", "pub_year": "2007", "author_list": "Arnaud, K. A.; Brown, D. A.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/zwsvh-vsm51", "eprint_id": 44547, "eprint_status": "archive", "datestamp": "2023-08-19 21:00:35", "lastmod": "2023-10-26 14:46:37", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D-C", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L", "name": { "family": "Goggin", "given": "L." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P-E", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Messaritaki-E", "name": { "family": "Messaritaki", "given": "E." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Tarallo-M", "name": { "family": "Tarallo", "given": "M." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "M." }, "orcid": "0000-0002-8107-5148" }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Search for gravitational wave radiation associated with the pulsating tail of the SGR 1806-20 hyperflare of 27 December 2004 using LIGO", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2007 American Physical Society. Received 9 April 2007. Published 27 September 2007. We are indebted to Gianluca Israel and Anna Watts for\nfrequent and fruitful discussions. The authors gratefully\nacknowledge the support of the United States National\nScience Foundation for the construction and operation of\nthe LIGO Laboratory and the Particle Physics and\nAstronomy Research Council of the United Kingdom, the\nMax-Planck-Society and the State of Niedersachsen/\nGermany for support of the construction and operation of\nthe GEO600 detector. The authors also gratefully acknowledge\nthe support of the research by these agencies and by\nthe Australian Research Council, the Natural Sciences and\nEngineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department\nof Science and Technology of India, the Spanish Ministerio\nde Educacion y Ciencia, the National Aeronautics and\nSpace Administration, the John Simon Guggenheim\nFoundation, the Alexander von Humboldt Foundation,\nthe Leverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation, the Alfred P.\nSloan Foundation, and Columbia University in New York\nCity.\n\nPublished - PhysRevD.76.062003.pdf
Submitted - 0703419v2.pdf
", "abstract": "We have searched for gravitational waves (GWs) associated with the SGR 1806\u221220 hyperflare of 27 December 2004. This event, originating from a Galactic neutron star, displayed exceptional energetics. Recent investigations of the x-ray light curve's pulsating tail revealed the presence of quasiperiodic oscillations (QPOs) in the 30\u20132000 Hz frequency range, most of which coincides with the bandwidth of the LIGO detectors. These QPOs, with well-characterized frequencies, can plausibly be attributed to seismic modes of the neutron star which could emit GWs. Our search targeted potential quasimonochromatic GWs lasting for tens of seconds and emitted at the QPO frequencies. We have observed no candidate signals above a predetermined threshold, and our lowest upper limit was set by the 92.5 Hz QPO observed in the interval from 150 s to 260 s after the start of the flare. This bound corresponds to a (90% confidence) root-sum-squared amplitude h^(90%)_(rss-det) =4.5\u00d710^(\u221222)\u2009\u2009strain\u2009\u2009Hz^(\u22121/2) on the GW waveform strength in the detectable polarization state reaching our Hanford (WA) 4 km detector. We illustrate the astrophysical significance of the result via an estimated characteristic energy in GW emission that we would expect to be able to detect. The above result corresponds to 7.7\u00d710^(46)\u2009\u2009erg (=4.3\u00d710^(\u22128)\u2009\u2009M_\u2299c^2), which is of the same order as the total (isotropic) energy emitted in the electromagnetic spectrum. This result provides a means to probe the energy reservoir of the source with the best upper limit on the GW waveform strength published and represents the first broadband asteroseismology measurement using a GW detector.", "date": "2007-09-27", "date_type": "published", "publication": "Physical Review D", "volume": "76", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 062003", "id_number": "CaltechAUTHORS:20140328-102903046", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140328-102903046", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada" }, { "agency": "Council of Scientific and Industrial Research of India" }, { "agency": "Spanish Ministerio de Educacion y Ciencia" }, { "agency": "NASA" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Alexander von Humboldt Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "New York City Columbia University" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.76.062003", "primary_object": { "basename": "PhysRevD.76.062003.pdf", "url": "https://authors.library.caltech.edu/records/zwsvh-vsm51/files/PhysRevD.76.062003.pdf" }, "related_objects": [ { "basename": "0703419v2.pdf", "url": "https://authors.library.caltech.edu/records/zwsvh-vsm51/files/0703419v2.pdf" } ], "resource_type": "article", "pub_year": "2007", "author_list": "Abbott, B.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/638z1-m4478", "eprint_id": 43374, "eprint_status": "archive", "datestamp": "2023-08-19 20:46:12", "lastmod": "2023-10-25 23:30:07", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Cepeda-C", "name": { "family": "Cepeda", "given": "C." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L-M", "name": { "family": "Goggin", "given": "L." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Messaritaki-E", "name": { "family": "Messaritaki", "given": "E." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Nocera-F", "name": { "family": "Nocera", "given": "F." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sanders-G-H", "name": { "family": "Sanders", "given": "G. H." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Tarallo-M", "name": { "family": "Tarallo", "given": "M." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Upper limits on gravitational wave emission from 78 radio pulsars", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2007 The American Physical Society. Received 4 April 2007; revised 20 June 2007; published 3 August 2007; publisher error corrected 29 February 2008. The authors gratefully acknowledge the support of the\nU.S. National Science Foundation for the construction and\noperation of the LIGO Laboratory, and the Particle Physics\nand Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/\nGermany for support of the construction and operation of\nthe GEO600 detector. The authors also gratefully acknowledge\nthe support of the research by these agencies and by\nthe Australian Research Council, the Natural Sciences and\nEngineering Research Council of Canada, the Council of\nScientific and Industrial Research of India, the Department\nof Science and Technology of India, the Spanish Ministerio\nde Educacion y Ciencia, the National Aeronautics and\nSpace Administration, the John Simon Guggenheim\nFoundation, the Alexander von Humboldt Foundation,\nthe Leverhulme Trust, the David and Lucile Packard\nFoundation, the Research Corporation, and the Alfred P.\nSloan Foundation.\n\nPublished - PhysRevD.76.042001.pdf
Submitted - 0702039v5.pdf
", "abstract": "We present upper limits on the gravitational wave emission from 78 radio pulsars based on data from the third and fourth science runs of the LIGO and GEO 600 gravitational wave detectors. The data from both runs have been combined coherently to maximize sensitivity. For the first time, pulsars within binary (or multiple) systems have been included in the search by taking into account the signal modulation due to their orbits. Our upper limits are therefore the first measured for 56 of these pulsars. For the remaining 22, our results improve on previous upper limits by up to a factor of 10. For example, our tightest upper limit on the gravitational strain is 2.6\u00d710^(\u221225) for PSR J1603\u22127202, and the equatorial ellipticity of PSR J2124\u20133358 is less than 10^(\u22126). Furthermore, our strain upper limit for the Crab pulsar is only 2.2 times greater than the fiducial spin-down limit.", "date": "2007-08-15", "date_type": "published", "publication": "Physical Review D", "volume": "76", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 042001", "id_number": "CaltechAUTHORS:20140115-091609260", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140115-091609260", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council of the United Kingdom" }, { "agency": "Max-Planck-Society and the State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada" }, { "agency": "Council of Scientific and Industrial Research of India" }, { "agency": "Department of Science and Technology of India" }, { "agency": "Spanish Ministerio de Educacion y Ciencia" }, { "agency": "NASA" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Alexander von Humboldt Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.76.042001", "primary_object": { "basename": "0702039v5.pdf", "url": "https://authors.library.caltech.edu/records/638z1-m4478/files/0702039v5.pdf" }, "related_objects": [ { "basename": "PhysRevD.76.042001.pdf", "url": "https://authors.library.caltech.edu/records/638z1-m4478/files/PhysRevD.76.042001.pdf" } ], "resource_type": "article", "pub_year": "2007", "author_list": "Abbott, B.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/qeaeh-ewc55", "eprint_id": 43372, "eprint_status": "archive", "datestamp": "2023-08-19 20:37:04", "lastmod": "2023-10-25 23:30:04", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Savov-P", "name": { "family": "Savov", "given": "P." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Boschi-V", "name": { "family": "Boschi", "given": "V." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. 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J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Espinoza-E", "name": { "family": "Espinoza", "given": "E." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Fairhurst-S", "name": { "family": "Fairhurst", "given": "S." } }, { "id": "Fazi-D", "name": { "family": "Fazi", "given": "D." } }, { "id": "Goggin-L", "name": { "family": "Goggin", "given": "L." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "Keppel-D-G", "name": { "family": "Keppel", "given": "D. G." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kondrashov-V", "name": { "family": "Kondrashov", "given": "V." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Marx-J-N", "name": { "family": "Marx", "given": "J. N." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Messaritaki-E", "name": { "family": "Messaritaki", "given": "E." } }, { "id": "Meyers-D", "name": { "family": "Meyers", "given": "D." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Patel-P", "name": { "family": "Patel", "given": "P." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Robertson-N-A", "name": { "family": "Robertson", "given": "N. A." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Samidi-M", "name": { "family": "Samidi", "given": "M." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Siemens-X", "name": { "family": "Siemens", "given": "X." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Tarallo-M", "name": { "family": "Tarallo", "given": "M." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Varvella-M", "name": { "family": "Varvella", "given": "M." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Villar-A", "name": { "family": "Villar", "given": "A." } }, { "id": "Waldman-S-J", "name": { "family": "Waldman", "given": "S. J." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "First cross-correlation analysis of interferometric and resonant-bar gravitational-wave data for stochastic backgrounds", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2007 The American Physical Society. Received 28 March 2007; published 9 July 2007; publisher error corrected 23 July 2007. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the\nParticle Physics and Astronomy Research Council of the\nUnited Kingdom, the Max-Planck-Society and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nNatural Sciences and Engineering Research Council of\nCanada, the Council of Scientific and Industrial Research\nof India, the Department of Science and Technology of\nIndia, the Spanish Ministerio de Educacion y Ciencia, The\nNational Aeronautics and Space Administration, the John\nSimon Guggenheim Foundation, the Alexander von\nHumboldt Foundation, the Leverhulme Trust, the David\nand Lucile Packard Foundation, the Research Corporation,\nand the Alfred P. Sloan Foundation. The ALLEGRO observatory\nis supported by the National Science Foundation,\nGrant No. PHY0215479. This paper has been assigned\nLIGO Document No. LIGO-P050020-09-Z.\n\nPublished - PhysRevD.76.022001.pdf
", "abstract": "Data from the LIGO Livingston interferometer and the ALLEGRO resonant-bar detector, taken during LIGO's fourth science run, were examined for cross correlations indicative of a stochastic gravitational-wave background in the frequency range 850\u2013950 Hz, with most of the sensitivity arising between 905 and 925 Hz. ALLEGRO was operated in three different orientations during the experiment to modulate the relative sign of gravitational-wave and environmental correlations. No statistically significant correlations were seen in any of the orientations, and the results were used to set a Bayesian 90% confidence level upper limit of \u03a9_(gw)(f)\u22641.02, which corresponds to a gravitational-wave strain at 915 Hz of 1.5\u00d710^(\u221223)\u2009\u2009Hz^(\u22121/2). In the traditional units of h^2_(100)\u03a9_(gw)(f), this is a limit of 0.53, 2 orders of magnitude better than the previous direct limit at these frequencies. The method was also validated with successful extraction of simulated signals injected in hardware and software.", "date": "2007-07-15", "date_type": "published", "publication": "Physical Review D", "volume": "76", "number": "2", "publisher": "American Physical Society", "pagerange": "Art. No. 022001", "id_number": "CaltechAUTHORS:20140115-080342758", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140115-080342758", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Astronomy Research Council (ARC)" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "NASA" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Alexander von Humboldt Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "NSF", "grant_number": "PHY-0215479" }, { "agency": "Max Planck Society" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P050020-09-Z", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration", "ALLEGRO Collaboration" ] }, "doi": "10.1103/PhysRevD.76.022001", "primary_object": { "basename": "PhysRevD.76.022001.pdf", "url": "https://authors.library.caltech.edu/records/qeaeh-ewc55/files/PhysRevD.76.022001.pdf" }, "resource_type": "article", "pub_year": "2007", "author_list": "Abbott, B.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/2r5ea-qsq59", "eprint_id": 43300, "eprint_status": "archive", "datestamp": "2023-08-19 20:03:47", "lastmod": "2023-10-25 23:26:38", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Barton-M-A", "name": { "family": "Barton", "given": "M. A." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. 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E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "C." } }, { "id": "Pan-Y", "name": { "family": "Pan", "given": "Y." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } } ] }, "title": "Searching for a Stochastic Background of Gravitational Waves with the Laser Interferometer Gravitational-Wave Observatory", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves", "note": "\u00a9 2007 American Astronomical Society. Received 2006 September 21; accepted 2006 November 30. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacion y Ciencia, The National Aeronautics\nand Space Administration, the John Simon Guggenheim\nFoundation, the Alexander von Humboldt Foundation, the\nLeverhulme Trust, the David and Lucile Packard Foundation,\nthe Research Corporation, and the Alfred P. Sloan Foundation.\nLIGO DCC number: P060012-07-D.\n\nPublished - 0004-637X_659_2_918.pdf
Submitted - 0608606v2.pdf
", "abstract": "The Laser Interferometer Gravitational-Wave Observatory (LIGO) has performed the fourth science run, S4, with significantly improved interferometer sensitivities with respect to previous runs. Using data acquired during this science run, we place a limit on the amplitude of a stochastic background of gravitational waves. For a frequency independent spectrum, the new Bayesian 90% upper limit is \u03a9_(GW) \u00d7 [H_0/(72 km s^(\u22121) Mpc^(\u22121))]^2 < 6.5 \u00d7 10^(-5). This is currently the most sensitive result in the frequency range 51-150 Hz, with a factor of 13 improvement over the previous LIGO result. We discuss the complementarity of the new result with other constraints on a stochastic background of gravitational waves, and we investigate implications of the new result for different models of this background.", "date": "2007-04-20", "date_type": "published", "publication": "Astrophysical Journal", "volume": "659", "number": "2", "publisher": "American Astronomical Society", "pagerange": "918-930", "id_number": "CaltechAUTHORS:20140110-072316825", "issn": "0004-637X", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140110-072316825", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "NASA" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Alexander von Humboldt Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "P060012-07-D", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1086/511329", "primary_object": { "basename": "0004-637X_659_2_918.pdf", "url": "https://authors.library.caltech.edu/records/2r5ea-qsq59/files/0004-637X_659_2_918.pdf" }, "related_objects": [ { "basename": "0608606v2.pdf", "url": "https://authors.library.caltech.edu/records/2r5ea-qsq59/files/0608606v2.pdf" } ], "resource_type": "article", "pub_year": "2007", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/patkc-gnx63", "eprint_id": 13777, "eprint_status": "archive", "datestamp": "2023-08-22 05:36:21", "lastmod": "2023-10-18 00:08:03", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "R." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Allen-J", "name": { "family": "Allen", "given": "J." } }, { "id": "Amin-R", "name": { "family": "Amin", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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"Ueda-A", "name": { "family": "Ueda, A", "given": "A." } }, { "id": "Waseda-K", "name": { "family": "Waseda", "given": "K." } }, { "id": "Yamamoto-A", "name": { "family": "Yamamoto", "given": "A." } }, { "id": "Yamamoto-K", "name": { "family": "Yamamoto", "given": "K." } }, { "id": "Yamazaki-T", "name": { "family": "Yamazaki", "given": "T." } }, { "id": "Yanagi-Y", "name": { "family": "Yanagi", "given": "Y." } }, { "id": "Yokoyama-J", "name": { "family": "Yokoyama", "given": "J." } }, { "id": "Yoshida-T", "name": { "family": "Yoshida", "given": "T." } }, { "id": "Zhu-Z-H", "name": { "family": "Zhu", "given": "Z.-H" } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Joint LIGO and TAMA300 search for gravitational waves from inspiralling neutron star binaries", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; neutron stars; binary stars; gravitational wave detectors; light interferometry", "note": "\u00a9 2006 The American Physical Society. \n\nReceived 11 January 2006; published 16 May 2006. \n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction and operation of the LIGO Laboratory and the\nParticle Physics and Astronomy Research Council of the\nUnited Kingdom, the Max-Planck-Society and the State of\nNiedersachsen/Germany for support of the construction\nand operation of the GEO600 detector. The authors also\ngratefully acknowledge the support of the research by these\nagencies and by the Australian Research Council, the\nNatural Sciences and Engineering Research Council of\nCanada, the Council of Scientific and Industrial Research\nof India, the Department of Science and Technology of\nIndia, the Spanish Ministerio de Educacion y Ciencia, the\nJohn Simon Guggenheim Foundation, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan Foundation. TAMA research is supported by a Grant-in- Aid for Scientific Research on Priority Areas (415) of the\nMinistry of Education, Culture, Sports, Science and\nTechnology of Japan. This work was also supported in\npart by JSPS Grant-in-Aid for Scientific Research\nNos. 14047214 and 12640269.\nPACS: \t 95.85.Sz; 04.80.Nn; 07.05.Kf; 95.55.Ym\n\nPublished - ABBprd06b.pdf
", "abstract": "We search for coincident gravitational wave signals from inspiralling neutron star binaries using LIGO and TAMA300 data taken during early 2003. Using a simple trigger exchange method, we perform an intercollaboration coincidence search during times when TAMA300 and only one of the LIGO sites were operational. We find no evidence of any gravitational wave signals. We place an observational upper limit on the rate of binary neutron star coalescence with component masses between 1 and 3M\u05e1\u05bc of 49 per year per Milky Way equivalent galaxy at a 90% confidence level. The methods developed during this search will find application in future network inspiral analyses.", "date": "2006-05", "date_type": "published", "publication": "Physical Review D", "volume": "73", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102002", "id_number": "CaltechAUTHORS:ABBprd06b", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd06b", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "Ministry of Education, Culture, Sports, Science and Technology (MEXT)" }, { "agency": "Japan Society for the Promotion of Science (JSPS)", "grant_number": "14047214" }, { "agency": "Japan Society for the Promotion of Science (JSPS)", "grant_number": "12640269" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.73.102002", "primary_object": { "basename": "ABBprd06b.pdf", "url": "https://authors.library.caltech.edu/records/patkc-gnx63/files/ABBprd06b.pdf" }, "resource_type": "article", "pub_year": "2006", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/bp84h-z8b47", "eprint_id": 13153, "eprint_status": "archive", "datestamp": "2023-08-19 17:29:21", "lastmod": "2023-10-17 21:47:52", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J" } }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Allen-J", "name": { "family": "Allen", "given": "J." } }, { "id": "Amin-R", "name": { "family": "Amin", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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J." } }, { "id": "Winkler-W", "name": { "family": "Winkler", "given": "W." } }, { "id": "Wise-S", "name": { "family": "Wise", "given": "S." } }, { "id": "Wiseman-A-G", "name": { "family": "Wiseman", "given": "A. G." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Woods-D", "name": { "family": "Woods", "given": "D." } }, { "id": "Wooley-R", "name": { "family": "Wooley", "given": "R." } }, { "id": "Worden-J", "name": { "family": "Worden", "given": "J." } }, { "id": "Wu-W", "name": { "family": "Wu", "given": "W." } }, { "id": "Yakushin-I", "name": { "family": "Yakushin", "given": "I." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yoshida-S", "name": { "family": "Yoshida", "given": "S." } }, { "id": "Zaleski-K-D", "name": { "family": "Zaleski", "given": "K. D." } }, { "id": "Zanolin-M", "name": { "family": "Zanolin", "given": "M." } }, { "id": "Zawischa-I", "name": { "family": "Zawischa", "given": "I." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zhu-R", "name": { "family": "Zhu", "given": "R." } }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for gravitational waves from binary black hole inspirals in LIGO data", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves, black holes, light interferometry", "note": "\u00a9 2006 The American Physical Society. \n\nReceived 26 October 2005; published 7 March 2006. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacion y Ciencia, the John Simon Guggenheim Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - ABBprd06a.pdf
Submitted - 0509129v1.pdf
", "abstract": "We report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20M_\u2609. Optimally oriented binaries with distances up to 1 Mpc could be detected with efficiency of at least 90%. We found no events that could be identified as gravitational waves in the 385.6 hours of data that we searched.", "date": "2006-03-07", "date_type": "published", "publication": "Physical Review D", "volume": "73", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 062001", "id_number": "CaltechAUTHORS:ABBprd06a", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd06a", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.73.062001", "primary_object": { "basename": "0509129v1.pdf", "url": "https://authors.library.caltech.edu/records/bp84h-z8b47/files/0509129v1.pdf" }, "related_objects": [ { "basename": "ABBprd06a.pdf", "url": "https://authors.library.caltech.edu/records/bp84h-z8b47/files/ABBprd06a.pdf" } ], "resource_type": "article", "pub_year": "2006", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/5y1ha-93249", "eprint_id": 13120, "eprint_status": "archive", "datestamp": "2023-08-22 04:43:14", "lastmod": "2023-10-17 21:47:20", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Ajith-P", "name": { "family": "Ajith", "given": "P." }, "orcid": "0000-0001-7519-2439" }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Allen-J", "name": { "family": "Allen", "given": "J." } }, { "id": "Amin-R", "name": { "family": "Amin", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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J." } }, { "id": "Winkler-W", "name": { "family": "Winkler", "given": "W." } }, { "id": "Wise-S", "name": { "family": "Wise", "given": "S." } }, { "id": "Wiseman-A-G", "name": { "family": "Wiseman", "given": "A. G." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Woods-D", "name": { "family": "Woods", "given": "D." } }, { "id": "Wooley-R", "name": { "family": "Wooley", "given": "R." } }, { "id": "Worden-J", "name": { "family": "Worden", "given": "J." } }, { "id": "Wu-W", "name": { "family": "Wu", "given": "W." } }, { "id": "Yakushin-I", "name": { "family": "Yakushin", "given": "I." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yoshida-S", "name": { "family": "Yoshida", "given": "S." } }, { "id": "Zaleski-K-D", "name": { "family": "Zaleski", "given": "K. D." } }, { "id": "Zanolin-M", "name": { "family": "Zanolin", "given": "M." } }, { "id": "Zawischa-I", "name": { "family": "Zawischa", "given": "I." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zhu-R", "name": { "family": "Zhu", "given": "R." } }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts", "ispublished": "pub", "full_text_status": "public", "keywords": "BLACK-HOLE COALESCENCES; CORE COLLAPSE; NETWORK", "note": "\u00a9 2005 The American Physical Society. \n\nReceived 8 August 2005; published 29 December 2005. \n\nThe LIGO scientific collaboration gratefully acknowledges the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacio\u00b4n y Ciencia, the John Simon Guggenheim Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. TAMA research is supported by a Grant-in-Aid for Scientific Research on Priority Areas (415) of the Japanese Ministry of Education, Culture, Sports, Science, and Technology. This document has been assigned LIGO Laboratory document No. LIGO-P040050-08-Z.\n\nPublished - ABBprd05f.pdf
", "abstract": "We report on the first joint search for gravitational waves by the TAMA and LIGO collaborations. We looked for millisecond-duration unmodeled gravitational-wave bursts in 473 hr of coincident data collected during early 2003. No candidate signals were found. We set an upper limit of 0.12 events per day on the rate of detectable gravitational-wave bursts, at 90% confidence level. From software simulations, we estimate that our detector network was sensitive to bursts with root-sum-square strain amplitude above approximately 1\u20133\u00d710-19\u2009\u2009Hz-1/2 in the frequency band 700-2000 Hz. We describe the details of this collaborative search, with particular emphasis on its advantages and disadvantages compared to searches by LIGO and TAMA separately using the same data. Benefits include a lower background and longer observation time, at some cost in sensitivity and bandwidth. We also demonstrate techniques for performing coincidence searches with a heterogeneous network of detectors with different noise spectra and orientations. These techniques include using coordinated software signal injections to estimate the network sensitivity, and tuning the analysis to maximize the sensitivity and the livetime, subject to constraints on the background.", "date": "2005-12-29", "date_type": "published", "publication": "Physical Review D", "volume": "72", "number": "12", "publisher": "American Physical Society", "pagerange": "Art. No. 122004", "id_number": "CaltechAUTHORS:ABBprd05", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd05", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "Ministry of Education, Culture, Sports, Science, and Technology (MEXT) of Japan" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P040050-08-Z", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "doi": "10.1103/PhysRevD.72.122004", "primary_object": { "basename": "ABBprd05f.pdf", "url": "https://authors.library.caltech.edu/records/5y1ha-93249/files/ABBprd05f.pdf" }, "resource_type": "article", "pub_year": "2005", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/vh0sz-5g221", "eprint_id": 23535, "eprint_status": "archive", "datestamp": "2023-08-19 16:41:28", "lastmod": "2023-10-23 19:44:06", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Barton-M-A", "name": { "family": "Barton", "given": "M. A." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Buonanno-A", "name": { "family": "Buonanno", "given": "A." } }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Charlton-P", "name": { "family": "Charlton", "given": "P." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Ehrens-P", "name": { "family": "Ehrens", "given": "P." } }, { "id": "Etzel-T", "name": { "family": "Etzel", "given": "T." } }, { "id": "Evans-M", "name": { "family": "Evans", "given": "M." } }, { "id": "Goggin-L", "name": { "family": "Goggin", "given": "L." } }, { "id": "Grimmett-D", "name": { "family": "Grimmett", "given": "D." } }, { "id": "Heefner-J", "name": { "family": "Heefner", "given": "J." } }, { "id": "Hoang-P", "name": { "family": "Hoang", "given": "P." } }, { "id": "Ivanov-A", "name": { "family": "Ivanov", "given": "A." } }, { "id": "Jones-L", "name": { "family": "Jones", "given": "L." } }, { "id": "Kells-W", "name": { "family": "Kells", "given": "W." } }, { "id": "King-P", "name": { "family": "King", "given": "P." } }, { "id": "Kozak-D-B", "name": { "family": "Kozak", "given": "D." }, "orcid": "0000-0003-3118-8950" }, { "id": "Lazzarini-A", "name": { "family": "Lazzarini", "given": "A." } }, { "id": "Lei-M", "name": { "family": "Lei", "given": "M." } }, { "id": "Libbrecht-K-G", "name": { "family": "Libbrecht", "given": "K." }, "orcid": "0000-0002-8744-3298" }, { "id": "Lindquist-P", "name": { "family": "Lindquist", "given": "P." } }, { "id": "Liu-S", "name": { "family": "Liu", "given": "S." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Mandic-V", "name": { "family": "Mandic", "given": "V." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Miyakawa-O", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Nocera-F", "name": { "family": "Nocera", "given": "F." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Romie-J", "name": { "family": "Romie", "given": "J." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Sanders-G-H", "name": { "family": "Sanders", "given": "G. H." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Shawhan-P", "name": { "family": "Shawhan", "given": "P." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Torrie-C", "name": { "family": "Torrie", "given": "C." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Wilson-A", "name": { "family": "Wilson", "given": "A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Pan-Y", "name": { "family": "Pan", "given": "Y." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" } ] }, "title": "Upper Limits on a Stochastic Background of Gravitational Waves", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2005 The American Physical Society. Received 30 July 2005; published 22 November 2005. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of Niedrersachsen, Germany, for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacion y Ciencia, the John Simon Guggenheim\nFoundation, the Leverhulme Trust, the David and Lucile\nPackard Foundation, the Research Corporation, and the\nAlfred P. Sloan Foundation.\n\nPublished - ABBprl05b.pdf
", "abstract": "The Laser Interferometer Gravitational-Wave Observatory has performed a third science run with much improved sensitivities of all three interferometers. We present an analysis of approximately 200 hours of data acquired during this run, used to search for a stochastic background of gravitational radiation. We place upper bounds on the energy density stored as gravitational radiation for three different spectral power laws. For the flat spectrum, our limit of \u03a9_0<8.4\u00d710^(-4) in the 69\u2013156 Hz band is ~10^5 times lower than the previous result in this frequency range.", "date": "2005-11-25", "date_type": "published", "publication": "Physical Review Letters", "volume": "95", "number": "22", "publisher": "American Physical Society", "pagerange": "Art. No. 221101", "id_number": "CaltechAUTHORS:20110503-140518412", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110503-140518412", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Max-Planck-Society" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educacion y Ciencia (MEC)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "State of Niedersachsen/Germany" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevLett.95.221101", "primary_object": { "basename": "ABBprl05b.pdf", "url": "https://authors.library.caltech.edu/records/vh0sz-5g221/files/ABBprl05b.pdf" }, "resource_type": "article", "pub_year": "2005", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/xqj0y-ytg86", "eprint_id": 23473, "eprint_status": "archive", "datestamp": "2023-08-19 16:34:38", "lastmod": "2023-10-23 19:36:56", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Agresti-J", "name": { "family": "Agresti", "given": "J." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Asiri-F", "name": { "family": "Asiri", "given": "F." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Barnes-M", "name": { "family": "Barnes", "given": "M." } }, { "id": "Barton-M-A", "name": { "family": "Barton", "given": "M. A." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. A." }, "orcid": "0000-0002-9180-5765" }, { "id": "Buonanno-A", "name": { "family": "Buonanno", "given": "A." } }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Chandler-A", "name": { "family": "Chandler", "given": "A." } }, { "id": "Chapsky-J", "name": { "family": "Chapsky", "given": "J." } }, { "id": "Charlton-P", "name": { "family": "Charlton", "given": "P." } }, { "id": "Chatterji-S", "name": { "family": "Chatterji", "given": "S." } }, { "id": "Coyne-D", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Ding-H", "name": { "family": "Ding", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Dupuis-R-J", "name": { "family": "Dupuis", "given": "R. J." } }, { "id": "Edlund-J-A", "name": { "family": "Edlund", "given": "J. 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H." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Schmidt-V", "name": { "family": "Schmidt", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Seel-S", "name": { "family": "Seel", "given": "S." } }, { "id": "Shawhan-P", "name": { "family": "Shawhan", "given": "P." } }, { "id": "Sievers-L", "name": { "family": "Sievers", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Spero-R", "name": { "family": "Spero", "given": "R." } }, { "id": "Sumner-M-C", "name": { "family": "Sumner", "given": "M. C." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Sylvestre-J", "name": { "family": "Sylvestre", "given": "J." } }, { "id": "Takamori-A", "name": { "family": "Takamori", "given": "A." } }, { "id": "Tariq-H", "name": { "family": "Tariq", "given": "H." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Tilav-S", "name": { "family": "Tilav", "given": "S." } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "M." }, "orcid": "0000-0002-8107-5148" }, { "id": "Torrie-C", "name": { "family": "Torrie", "given": "C." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ward-R", "name": { "family": "Ward", "given": "R." } }, { "id": "Ware-B", "name": { "family": "Ware", "given": "B." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Williams-R", "name": { "family": "Williams", "given": "R." } }, { "id": "Wilson-A", "name": { "family": "Wilson", "given": "A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" } ] }, "title": "First all-sky upper limits from LIGO on the strength of periodic gravitational waves using the Hough transform", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2005 The American Physical Society. Received 13 September 2005; published 28 November 2005. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educaci\u03ccn y Ciencia, the\nJohn Simon Guggenheim Foundation, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory document number LIGOP050013-00-R.\n\nPublished - ABBprd05e.pdf
", "abstract": "We perform a wide parameter-space search for continuous gravitational waves over the whole sky and over a large range of values of the frequency and the first spin-down parameter. Our search method is based on the Hough transform, which is a semicoherent, computationally efficient, and robust pattern recognition technique. We apply this technique to data from the second science run of the LIGO detectors and our final results are all-sky upper limits on the strength of gravitational waves emitted by unknown isolated spinning neutron stars on a set of narrow frequency bands in the range 200\u2013400\u2009\u200a\u200aHz. The best upper limit on the gravitational-wave strain amplitude that we obtain in this frequency range is 4.43\u00d710^(-23).", "date": "2005-11", "date_type": "published", "publication": "Physical Review D", "volume": "72", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102004", "id_number": "CaltechAUTHORS:20110426-152707978", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110426-152707978", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Max-Planck-Society" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia (MEC)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "State of Niedersachsen/Germany" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P050013-00R", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.72.102004", "primary_object": { "basename": "ABBprd05e.pdf", "url": "https://authors.library.caltech.edu/records/xqj0y-ytg86/files/ABBprd05e.pdf" }, "resource_type": "article", "pub_year": "2005", "author_list": "Abbott, B.; Adhikari, Rana X.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/pmeep-m8415", "eprint_id": 1897, "eprint_status": "archive", "datestamp": "2023-08-22 04:18:26", "lastmod": "2023-10-13 23:04:29", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Buonanno-A", "name": { "family": "Buonanno", "given": "Alessandra" } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Yanbei" }, "orcid": "0000-0002-9730-9463" }, { "id": "Pan-Y", "name": { "family": "Pan", "given": "Yi" } }, { "id": "Tagoshi-H", "name": { "family": "Tagoshi", "given": "Hideyuki" } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Detecting gravitational waves from precessing binaries of spinning compact objects. II. Search implementation for low-mass binaries", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational waves; binary stars; stellar mass; black holes; neutron stars", "note": "\u00a92005 The American Physical Society \n\n(Received 22 August 2005; published 26 October 2005) \n\nWe thank B. S. Sathyaprakash for useful discussions, and the LSC internal referee for providing valuable comments. M.V. is grateful to the LISA group at APC-Colle`ge de France for hospitality during the completion of this work. Research that led to this paper was supported by NSF Grant No. PHY-0099568; Y. C.'s research was also supported by the David and Barbara Groce Fund at the San Diego Foundation, and by the Alexander von Humboldt Foundation Sofja Kovalevskaja Program, funded by the German Federal Ministry of Education and Research; M.V.'s research was also supported by the LISA Mission Science Office at the Jet Propulsion Laboratory, California Institute of Technology, where it was performed under contract with the National Aeronautics and Space Administration; H. T.'s research was partially supported by Grants-in-Aid for Scientific Research (No. 14047214, No. 12640269, and No. 16540251) at the Ministry of Education of Japan.", "abstract": "Detection template families (DTFs) are built to capture the essential features of true gravitational waveforms using a small set of phenomenological waveform parameters. Buonanno, Chen, and Vallisneri [Phys. Rev. D 67, 104025 (2003)] proposed the BCV2 DTF to perform computationally efficient searches for signals from precessing binaries of compact stellar objects. Here we test the signal-matching performance of the BCV2 DTF for asymmetric-mass-ratio binaries, and specifically for double-black-hole binaries with component masses (m1,m2)[is-an-element-of][6,12]M[sun]\u00d7[1,3]M[sun], and for black-hole\u2013neutron-star binaries with component masses (m1,m2)=(10M[sun],1.4M[sun]); we take all black holes to be maximally spinning. We find a satisfactory signal-matching performance, with fitting factors averaging between 0.94 and 0.98. We also scope out the region of BCV2 parameters needed for a template-based search, we evaluate the template match metric, we discuss a template-placement strategy, and we estimate the number of templates needed for searches at the LIGO design sensitivity. In addition, after gaining more insight in the dynamics of spin-orbit precession, we propose a modification of the BCV2 DTF that is parametrized by physical (rather than phenomenological) parameters. We test this modified \"BCV2P\" DTF for the (10M[sun], 1.4M[sun]) black-hole\u2013neutron-star system, finding a signal-matching performance comparable to the BCV2 DTF, and a reliable parameter-estimation capability for target-binary quantities such as the chirp mass and the opening angle (the angle between the black-hole spin and the orbital angular momentum).", "date": "2005-10-15", "date_type": "published", "publication": "Physical Review D", "volume": "72", "number": "8", "publisher": "American Physical Society", "pagerange": "Art. No. 084027", "id_number": "CaltechAUTHORS:BUOprd05", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:BUOprd05", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1103/PhysRevD.72.084027", "primary_object": { "basename": "BUOprd05.pdf", "url": "https://authors.library.caltech.edu/records/pmeep-m8415/files/BUOprd05.pdf" }, "resource_type": "article", "pub_year": "2005", "author_list": "Buonanno, Alessandra; Chen, Yanbei; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/sp5dm-yyy36", "eprint_id": 13104, "eprint_status": "archive", "datestamp": "2023-08-19 16:31:47", "lastmod": "2023-10-17 21:46:48", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. P." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Amin-R", "name": { "family": "Amin", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Anderson-W-G", "name": { "family": "Anderson", "given": "W. G." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Ashley-M-C-B", "name": { "family": "Ashley", "given": "M." } }, { "id": "Asiri-F", "name": { "family": "Asiri", "given": "F." } }, { "id": "Aufmuth-P", "name": { "family": "Aufmuth", "given": "P." } }, { "id": "Aulbert-C", "name": { "family": "Aulbert", "given": "C." } }, { "id": "Babak-S", "name": { "family": "Babak", "given": "S." } }, { "id": "Balasubramanian-R", "name": { "family": "Balasubramanian", "given": "R." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Barker-C", "name": { "family": "Barker", "given": "C." } }, { "id": "Barker-D", "name": { "family": "Barker", "given": "D." } }, { "id": "Barnes-M", "name": { "family": "Barnes", "given": "M." } }, { "id": "Barr-B", "name": { "family": "Barr", "given": "B." } }, { "id": "Barton-M-A", "name": { "family": "Barton", "given": "M. A." } }, { "id": "Bayer-K", "name": { "family": "Bayer", "given": "K." } }, { "id": "Beausoleil-R", "name": { "family": "Beausoleil", "given": "R." } }, { "id": "Belczynski-K", "name": { "family": "Belczynski", "given": "K." } }, { "id": "Bennett-R", "name": { "family": "Bennett", "given": "R." } }, { "id": "Berukoff-S-J", "name": { "family": "Berukoff", "given": "S. J." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Bilenko-I-A", "name": { "family": "Bilenko", "given": "I. A." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Blackburn-L", "name": { "family": "Blackburn", "given": "L." } }, { "id": "Bland-B", "name": { "family": "Bland", "given": "B." } }, { "id": "Bochner-B", "name": { "family": "Bochner", "given": "B." } }, { "id": "Bogue-L", "name": { "family": "Bogue", "given": "L." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Bose-Sukanta", "name": { "family": "Bose", "given": "S." }, "orcid": "0000-0002-3445-4479" }, { "id": "Brady-P-R", "name": { "family": "Brady", "given": "P. R." }, "orcid": "0000-0002-4611-9387" }, { "id": "Braginsky-V-B", "name": { "family": "Braginsky", "given": "V. B." } }, { "id": "Brau-J-E", "name": { "family": "Brau", "given": "J. 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D." } }, { "id": "Zanolin-M", "name": { "family": "Zanolin", "given": "M." } }, { "id": "Zawischa-I", "name": { "family": "Zawischa", "given": "I." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zhu-R", "name": { "family": "Zhu", "given": "R." } }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for gravitational waves from galactic and extra-galactic binary neutron stars", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2005 American Physical Society. \n\nReceived 30 May 2005; published 25 October 2005. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacion y Ciencia, the John Simon Guggenheim Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - ABBprd05d.pdf
", "abstract": "We use 373 hours (\u224815 days) of data from the second science run of the LIGO gravitational-wave detectors to search for signals from binary neutron star coalescences within a maximum distance of about 1.5 Mpc, a volume of space which includes the Andromeda Galaxy and other galaxies of the Local Group of galaxies. This analysis requires a signal to be found in data from detectors at the two LIGO sites, according to a set of coincidence criteria. The background (accidental coincidence rate) is determined from the data and is used to judge the significance of event candidates. No inspiral gravitational-wave events were identified in our search. Using a population model which includes the Local Group, we establish an upper limit of less than 47 inspiral events per year per Milky Way equivalent galaxy with 90% confidence for nonspinning binary neutron star systems with component masses between 1 and 3M\u2609.", "date": "2005-10-15", "date_type": "published", "publication": "Physical Review D", "volume": "72", "number": "8", "publisher": "American Physical Society", "pagerange": "Art. No. 082001", "id_number": "CaltechAUTHORS:ABBprd05d", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd05d", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "doi": "10.1103/PhysRevD.72.082001", "primary_object": { "basename": "ABBprd05d.pdf", "url": "https://authors.library.caltech.edu/records/sp5dm-yyy36/files/ABBprd05d.pdf" }, "resource_type": "article", "pub_year": "2005", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/sg472-58d56", "eprint_id": 13074, "eprint_status": "archive", "datestamp": "2023-08-19 16:31:39", "lastmod": "2023-10-17 21:45:36", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Amin-R", "name": { "family": "Amin", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Anderson-W-G", "name": { "family": "Anderson", "given": "W. 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Y." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zhu-R", "name": { "family": "Zhu", "given": "R." } }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Search for gravitational waves from primordial black hole binary coalescences in the galactic halo", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2005 American Physical Society. \n\nReceived 30 May 2005; published 25 October 2005. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Ciencia y Tecnologia, the John Simon Guggenheim Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - ABBprd05c.pdf
", "abstract": "We use data from the second science run of the LIGO gravitational-wave detectors to search for the gravitational waves from primordial black hole binary coalescence with component masses in the range 0.2\u20131.0M\u2609. The analysis requires a signal to be found in the data from both LIGO observatories, according to a set of coincidence criteria. No inspiral signals were found. Assuming a spherical halo with core radius 5 kpc extending to 50 kpc containing nonspinning black holes with masses in the range 0.2\u20131.0M\u2609, we place an observational upper limit on the rate of primordial black hole coalescence of 63 per year per Milky Way halo (MWH) with 90% confidence.", "date": "2005-10-15", "date_type": "published", "publication": "Physical Review D", "volume": "72", "number": "8", "publisher": "American Physical Society", "pagerange": "Art. No. 082002", "id_number": "CaltechAUTHORS:ABBprd05c", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd05c", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.72.082002", "primary_object": { "basename": "ABBprd05c.pdf", "url": "https://authors.library.caltech.edu/records/sg472-58d56/files/ABBprd05c.pdf" }, "resource_type": "article", "pub_year": "2005", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/0k97z-xav94", "eprint_id": 13020, "eprint_status": "archive", "datestamp": "2023-08-22 04:11:21", "lastmod": "2023-10-17 21:42:59", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B. 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D." } }, { "id": "Zanolin-M", "name": { "family": "Zanolin", "given": "M." } }, { "id": "Zawischa-I", "name": { "family": "Zawischa", "given": "I." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zhu-R", "name": { "family": "Zhu", "given": "R." } }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Upper limits on gravitational wave bursts in LIGO's second science run", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational wave detectors; gravitational waves; light interferometry; time-frequency analysis; waveform analysis", "note": "\u00a9 2005 American Physical Society. \n\nReceived 7 June 2005; published 8 September 2005. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Educacion y Ciencia, the John Simon Guggenheim Foundation, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory document number LIGO-P040040-A-R.\n\nPublished - ABBprd05b.pdf
", "abstract": "We perform a search for gravitational wave bursts using data from the second science run of the LIGO detectors, using a method based on a wavelet time-frequency decomposition. This search is sensitive to bursts of duration much less than a second and with frequency content in the 100\u20131100 Hz range. It features significant improvements in the instrument sensitivity and in the analysis pipeline with respect to the burst search previously reported by LIGO. Improvements in the search method allow exploring weaker signals, relative to the detector noise floor, while maintaining a low false alarm rate, O(0.1) \u03bcHz. The sensitivity in terms of the root-sum-square (rss) strain amplitude lies in the range of hrss\u223c10^-20 - 10^-19\u2009\u2009Hz^-1/2. No gravitational wave signals were detected in 9.98 days of analyzed data. We interpret the search result in terms of a frequentist upper limit on the rate of detectable gravitational wave bursts at the level of 0.26 events per day at 90% confidence level. We combine this limit with measurements of the detection efficiency for selected waveform morphologies in order to yield rate versus strength exclusion curves as well as to establish order-of-magnitude distance sensitivity to certain modeled astrophysical sources. Both the rate upper limit and its applicability to signal strengths improve our previously reported limits and reflect the most sensitive broad-band search for untriggered and unmodeled gravitational wave bursts to date.", "date": "2005-09-15", "date_type": "published", "publication": "Physical Review D", "volume": "72", "number": "6", "publisher": "American Physical Society", "pagerange": "Art. No. 062001", "id_number": "CaltechAUTHORS:ABBprd05b", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd05b", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P040040-A-R", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.72.062001", "primary_object": { "basename": "ABBprd05b.pdf", "url": "https://authors.library.caltech.edu/records/0k97z-xav94/files/ABBprd05b.pdf" }, "resource_type": "article", "pub_year": "2005", "author_list": "Abbott, B. P.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/rf493-jrs51", "eprint_id": 43369, "eprint_status": "archive", "datestamp": "2023-08-19 16:08:57", "lastmod": "2023-10-25 23:30:01", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. 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J." } }, { "id": "Sylvestre-J", "name": { "family": "Sylvestre", "given": "J." } }, { "id": "Takamori-A", "name": { "family": "Takamori", "given": "A." } }, { "id": "Tariq-H", "name": { "family": "Tariq", "given": "H." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tilav-S", "name": { "family": "Tilav", "given": "S." } }, { "id": "Torrie-C", "name": { "family": "Torrie", "given": "C." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ware-B", "name": { "family": "Ware", "given": "B." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Wilson-A", "name": { "family": "Wilson", "given": "A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Search for gravitational waves associated with the gamma ray burst GRB030329 using the LIGO detectors", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2005 The American Physical Society. Received 21 February 2005; published 12 August 2005. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Ciencia y Tecnologia, the John Simon Guggenheim Foundation, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan Foundation.\nWe are grateful to Scott Barthelmy and the GCN network and Kevin Hurley and the IPN network for providing us with near real time GRB triggers and to the Ulysses, Konus, SAX, and HETE experiments, who detect and generate the events distributed by GCN and IPN. This research has made use of data obtained from the HETE science team via the website in Ref. [75]. HETE is an international mission of the NASA Explorer program, run by the Massachusetts Institute of Technology.\n\nPublished - PhysRevD.72.042002.pdf
", "abstract": "We have performed a search for bursts of gravitational waves associated with the very bright gamma ray burst GRB030329, using the two detectors at the LIGO Hanford Observatory. Our search covered the most sensitive frequency range of the LIGO detectors (approximately 80\u2013\u22122048\u2009\u200a\u200aHz), and we specifically targeted signals shorter than \u2243150\u2009\u2009ms. Our search algorithm looks for excess correlated power between the two interferometers and thus makes minimal assumptions about the gravitational waveform. We observed no candidates with gravitational-wave signal strength larger than a predetermined threshold. We report frequency-dependent upper limits on the strength of the gravitational waves associated with GRB030329. Near the most sensitive frequency region, around \u2243250\u2009\u2009Hz, our root-sum-square (RSS) gravitational-wave strain sensitivity for optimally polarized bursts was better than h_(RSS)\u22436\u00d710^(\u221221)\u2009\u2009Hz^(\u22121/2). Our result is comparable to the best published results searching for association between gravitational waves and gamma ray bursts.", "date": "2005-08", "date_type": "published", "publication": "Physical Review D", "volume": "72", "number": "4", "publisher": "American Physical Society", "pagerange": "Art. No. 042002", "id_number": "CaltechAUTHORS:20140114-151827275", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140114-151827275", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (United Kingdom)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Ciencia y Tecnologia (MCYT)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.72.042002", "primary_object": { "basename": "PhysRevD.72.042002.pdf", "url": "https://authors.library.caltech.edu/records/rf493-jrs51/files/PhysRevD.72.042002.pdf" }, "resource_type": "article", "pub_year": "2005", "author_list": "Abbott, B.; Drever, R. W. P.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/awe59-3r584", "eprint_id": 23531, "eprint_status": "archive", "datestamp": "2023-08-19 15:46:27", "lastmod": "2023-10-23 19:43:55", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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A." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bogue-L", "name": { "family": "Bogue", "given": "L." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Buonanno-A", "name": { "family": "Buonanno", "given": "A." } }, { "id": "Busby-D", "name": { "family": "Busby", "given": "D." } }, { "id": "Cardenas-L", "name": { "family": "Cardenas", "given": "L." } }, { "id": "Chandler-A", "name": { "family": "Chandler", "given": "A." } }, { "id": "Chapsky-J", "name": { "family": "Chapsky", "given": "J." } }, { "id": "Charlton-P", "name": { "family": "Charlton", "given": "P." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Coyne-D", "name": { "family": "Coyne", "given": "D." }, "orcid": "0000-0002-6427-3222" }, { "id": "Creighton-T-D", "name": { "family": "Creighton", "given": "T. D." } }, { "id": "D'Ambrosio-E", "name": { "family": "D'Ambrosio", "given": "E." } }, { "id": "DeSalvo-R", "name": { "family": "DeSalvo", "given": "R." } }, { "id": "Ding-H", "name": { "family": "Ding", "given": "H." } }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Edlund-J-A", "name": { "family": "Edlund", "given": "J. 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T." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Majid-W", "name": { "family": "Majid", "given": "W." } }, { "id": "Mann-F", "name": { "family": "Mann", "given": "F." } }, { "id": "M\u00e1rka-S", "name": { "family": "M\u00e1rka", "given": "S." } }, { "id": "Maros-E", "name": { "family": "Maros", "given": "E." } }, { "id": "Mason-J", "name": { "family": "Mason", "given": "J." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Miyoki-S", "name": { "family": "Miyoki", "given": "S." } }, { "id": "Nash-T", "name": { "family": "Nash", "given": "T." } }, { "id": "Nocera-F", "name": { "family": "Nocera", "given": "F." } }, { "id": "Ouimette-D", "name": { "family": "Ouimette", "given": "D." } }, { "id": "Pan-Y", "name": { "family": "Pan", "given": "Y." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Rao-S-R", "name": { "family": "Rao", "given": "S. R." } }, { "id": "Redding-D", "name": { "family": "Redding", "given": "D." } }, { "id": "Regehr-M-W", "name": { "family": "Regehr", "given": "M. W." } }, { "id": "Reilly-K-T", "name": { "family": "Reilly", "given": "K. T." } }, { "id": "Reithmaier-K", "name": { "family": "Reithmaier", "given": "K." } }, { "id": "Robison-L", "name": { "family": "Robison", "given": "L." } }, { "id": "Romie-J", "name": { "family": "Romie", "given": "J." } }, { "id": "Rose-D", "name": { "family": "Rose", "given": "D." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Salzman-I", "name": { "family": "Salzman", "given": "I." } }, { "id": "Sanders-G-H", "name": { "family": "Sanders", "given": "G. H." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Seel-S", "name": { "family": "Seel", "given": "S." } }, { "id": "Shawhan-P", "name": { "family": "Shawhan", "given": "P." } }, { "id": "Sievers-L", "name": { "family": "Sievers", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Spero-R", "name": { "family": "Spero", "given": "R." } }, { "id": "Sumner-M-C", "name": { "family": "Sumner", "given": "M. C." } }, { "id": "Sutton-P-J", "name": { "family": "Sutton", "given": "P. J." } }, { "id": "Sylvestre-J", "name": { "family": "Sylvestre", "given": "J." } }, { "id": "Takamori-A", "name": { "family": "Takamori", "given": "A." } }, { "id": "Tariq-H", "name": { "family": "Tariq", "given": "H." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Tilav-S", "name": { "family": "Tilav", "given": "S." } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "M." }, "orcid": "0000-0002-8107-5148" }, { "id": "Torrie-C", "name": { "family": "Torrie", "given": "C." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ware-B", "name": { "family": "Ware", "given": "B." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wilson-A", "name": { "family": "Wilson", "given": "A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Limits on Gravitational-Wave Emission from Selected Pulsars Using LIGO Data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2005 The American Physical Society. Received 29 October 2004; published 12 May 2005. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Ciencia y Tecnologia, the John Simon Guggenheim Foundation, the Leverhulme\nTrust, the David and Lucile Packard Foundation, the\nResearch Corporation, and the Alfred P. Sloan Foundation. This document has been assigned LIGO Laboratory Document No. LIGO-P040008-C-Z.\n\nPublished - ABBprl05a.pdf
", "abstract": "We place direct upper limits on the amplitude of gravitational waves from 28 isolated radio pulsars by a coherent multidetector analysis of the data collected during the second science run of the LIGO interferometric detectors. These are the first direct upper limits for 26 of the 28 pulsars. We use coordinated radio observations for the first time to build radio-guided phase templates for the expected gravitational-wave signals. The unprecedented sensitivity of the detectors allows us to set strain upper limits as low as a few times 10^(-24). These strain limits translate into limits on the equatorial ellipticities of the pulsars, which are smaller than 10^(-5) for the four closest pulsars.", "date": "2005-05-13", "date_type": "published", "publication": "Physical Review Letters", "volume": "94", "number": "18", "publisher": "American Physical Society", "pagerange": "Art. No. 181103", "id_number": "CaltechAUTHORS:20110503-112854281", "issn": "0031-9007", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110503-112854281", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Max-Planck-Society" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Ciencia y Tecnologia (MCYT)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "Leverhulme Trust" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "State of Niedersachsen/Germany" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P040008-C-Z", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevLett.94.181103", "primary_object": { "basename": "ABBprl05a.pdf", "url": "https://authors.library.caltech.edu/records/awe59-3r584/files/ABBprl05a.pdf" }, "resource_type": "article", "pub_year": "2005", "author_list": "Abbott, B.; Anderson, S. B.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/fqw5z-31w81", "eprint_id": 4890, "eprint_status": "archive", "datestamp": "2023-08-22 02:35:59", "lastmod": "2023-10-16 17:59:20", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Gair-J-R", "name": { "family": "Gair", "given": "Jonathan R." } }, { "id": "Barack-L", "name": { "family": "Barack", "given": "Leor" } }, { "id": "Creighton-T", "name": { "family": "Creighton", "given": "Teviet" } }, { "id": "Cutler-C-J", "name": { "family": "Cutler", "given": "Curt" } }, { "id": "Larson-S-L", "name": { "family": "Larson", "given": "Shane L." } }, { "id": "Phinney-E-S", "name": { "family": "Phinney", "given": "E. Sterl" } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Event rate estimates for LISA extreme mass ratio capture sources", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2006 IOP Publishing Limited \n\nReceived 3 April 2004; Published 24 September 2004; Print publication: Issue 20 (21 October 2004) \n\nThis work would not have been possible without the guidance and encouragement of Kip Thorne, who repeatedly cracked the whip to make sure the project stayed on schedule. We also thank Kostas Glampedakis, Scott Hughes and Daniel Kennefick for the use of their kludge waveform code and for many useful discussions at EMRI telecons. This work was supported in part by NASA grants NAG5-12834 (CC, JG) and NAG5-10707 (JG, ESP), LISA contract number PO 1217163 (SL, TC), a Marie Curie Fellowship of the European Community program IHP-MCIF-99-1 under contract number HPMF-CT-2000-00851 (LB), NSF Grant NSF-PHY-0140326 ('Kudu') (LB), a grant from NASA-URC-Brownsville (LB) and by the LISA Mission Science office at JPL under contract with NASA (MV). \n\nSPECIAL ISSUE: PROCEEDINGS OF THE 8TH GRAVITATIONAL WAVE DATA ANALYSIS WORKSHOP, MILWAUKEE, WI, USA, 17-20 DECEMBER 2003\n\nPublished - GAIcqg04.pdf
Submitted - 0405137
", "abstract": "One of the most exciting prospects for the LISA gravitational wave observatory is the detection of gravitational radiation from the inspiral of a compact object into a supermassive black hole. The large inspiral parameter space and low amplitude of the signal make detection of these sources computationally challenging. We outline here a first-cut data analysis scheme that assumes realistic computational resources. In the context of this scheme, we estimate the signal-to-noise ratio that a source requires to pass our thresholds and be detected. Combining this with an estimate of the population of sources in the universe, we estimate the number of inspiral events that LISA could detect. The preliminary results are very encouraging\u2014with the baseline design, LISA can see inspirals out to a redshift z = 1 and should detect over a thousand events during the mission lifetime.", "date": "2004-10-21", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "21", "number": "20", "publisher": "IOP", "pagerange": "S1595-S1606", "id_number": "CaltechAUTHORS:GAIcqg04", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:GAIcqg04", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1088/0264-9381/21/20/003", "primary_object": { "basename": "0405137", "url": "https://authors.library.caltech.edu/records/fqw5z-31w81/files/0405137" }, "related_objects": [ { "basename": "GAIcqg04.pdf", "url": "https://authors.library.caltech.edu/records/fqw5z-31w81/files/GAIcqg04.pdf" } ], "resource_type": "article", "pub_year": "2004", "author_list": "Gair, Jonathan R.; Barack, Leor; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/cv6cd-8rw91", "eprint_id": 76231, "eprint_status": "archive", "datestamp": "2023-08-19 13:56:45", "lastmod": "2023-10-20 22:05:54", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Kr\u00f3lak-A", "name": { "family": "Kr\u00f3lak", "given": "Andrzej" } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "Massimo" }, "orcid": "0000-0002-8107-5148" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Optimal filtering of the LISA data", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2004 American Physical Society. \n\n(Received 19 January 2004; published 26 July 2004) \n\nA.K. acknowledges support from the National Research Council at the Jet Propulsion Laboratory, Caltech. M.V.'s research was supported by the LISA Mission Science Office at the Jet Propulsion Laboratory, Caltech. This research was performed at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.\n\nErratum: Optimal filtering of the LISA data [Phys. Rev. D 70, 022003 (2004)]\nAndrzej Kr\u00f3lak, Massimo Tinto, and Michele Vallisneri\nPhys. Rev. D 76, 069901\n\nAccepted Version - 0401108.pdf
Erratum - PhysRevD.70.022003.pdf
", "abstract": "The LISA time-delay-interferometry responses to a gravitational wave signal are rewritten in a form that accounts for the motion of the LISA constellation around the Sun; the responses are given in closed analytic forms valid for any frequency in the band accessible to LISA. We then present a complete procedure, based on the principle of maximum likelihood, to search for stellar-mass binary systems in the LISA data. We define the required optimal filters, the amplitude-maximized detection statistic (analogous to the \u0191 statistic used in pulsar searches with ground-based interferometers), and discuss the false-alarm and detection probabilities. We then test the procedure in numerical simulations of gravitational-wave detection.", "date": "2004-07-15", "date_type": "published", "publication": "Physical Review D", "volume": "70", "number": "2", "publisher": "American Physical Society", "pagerange": "Art. No. 022003", "id_number": "CaltechAUTHORS:20170408-164051256", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170408-164051256", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "National Research Council" }, { "agency": "NASA/JPL/Caltech" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "doi": "10.1103/PhysRevD.70.022003", "primary_object": { "basename": "PhysRevD.70.022003.pdf", "url": "https://authors.library.caltech.edu/records/cv6cd-8rw91/files/PhysRevD.70.022003.pdf" }, "related_objects": [ { "basename": "0401108.pdf", "url": "https://authors.library.caltech.edu/records/cv6cd-8rw91/files/0401108.pdf" } ], "resource_type": "article", "pub_year": "2004", "author_list": "Kr\u00f3lak, Andrzej; Tinto, Massimo; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/fyg3m-x4t84", "eprint_id": 12975, "eprint_status": "archive", "datestamp": "2023-08-22 02:04:22", "lastmod": "2023-10-17 21:41:09", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Amin-R", "name": { "family": "Amin", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. B." } }, { "id": "Anderson-W-G", "name": { "family": "Anderson", "given": "W. G." } }, { "id": "Araya-M", "name": { "family": "Araya", "given": "M." } }, { "id": "Armandula-H", "name": { "family": "Armandula", "given": "H." } }, { "id": "Asiri-F", "name": { "family": "Asiri", "given": "F." } }, { "id": "Aufmuth-P", "name": { "family": "Aufmuth", "given": "P." } }, { "id": "Aulbert-C", "name": { "family": "Aulbert", "given": "C." } }, { "id": "Babak-S", "name": { "family": "Babak", "given": "S." } }, { "id": "Balasubramanian-R", "name": { "family": "Balasubramanian", "given": "R." } }, { "id": "Ballmer-S", "name": { "family": "Ballmer", "given": "S." } }, { "id": "Barish-B-C", "name": { "family": "Barish", "given": "B. C." } }, { "id": "Barker-D", "name": { "family": "Barker", "given": "D." } }, { "id": "Barker-Patton-C", "name": { "family": "Barker-Patton", "given": "C." } }, { "id": "Barnes-M", "name": { "family": "Barnes", "given": "M." } }, { "id": "Barr-B", "name": { "family": "Barr", "given": "B." } }, { "id": "Barton-M-A", "name": { "family": "Barton", "given": "M. A." } }, { "id": "Bayer-K", "name": { "family": "Bayer", "given": "K." } }, { "id": "Beausoleil-R", "name": { "family": "Beausoleil", "given": "R." } }, { "id": "Belczynski-K", "name": { "family": "Belczynski", "given": "K." } }, { "id": "Bennett-R", "name": { "family": "Bennett", "given": "R." } }, { "id": "Berukoff-S-J", "name": { "family": "Berukoff", "given": "S. J." } }, { "id": "Betzwieser-J", "name": { "family": "Betzwieser", "given": "J." } }, { "id": "Bhawal-B", "name": { "family": "Bhawal", "given": "B." } }, { "id": "Bilenko-I-A", "name": { "family": "Bilenko", "given": "I. A." } }, { "id": "Billingsley-G", "name": { "family": "Billingsley", "given": "G." }, "orcid": "0000-0002-4141-2744" }, { "id": "Black-E", "name": { "family": "Black", "given": "E." } }, { "id": "Blackburn-K", "name": { "family": "Blackburn", "given": "K." } }, { "id": "Bland-Weaver-B", "name": { "family": "Bland-Weaver", "given": "B." } }, { "id": "Bochner-B", "name": { "family": "Bochner", "given": "B." } }, { "id": "Bogue-L", "name": { "family": "Bogue", "given": "L." } }, { "id": "Bork-R", "name": { "family": "Bork", "given": "R." } }, { "id": "Bose-Sukanta", "name": { "family": "Bose", "given": "S." }, "orcid": "0000-0002-3445-4479" }, { "id": "Brady-P-R", "name": { "family": "Brady", "given": "P. R." }, "orcid": "0000-0002-4611-9387" }, { "id": "Braginsky-V-B", "name": { "family": "Braginsky", "given": "V. B." } }, { "id": "Brau-J-E", "name": { "family": "Brau", "given": "J. E." } }, { "id": "Brown-D-A", "name": { "family": "Brown", "given": "D. 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G." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Wooley-R", "name": { "family": "Wooley", "given": "R." } }, { "id": "Worden-J", "name": { "family": "Worden", "given": "J." } }, { "id": "Yakushin-I", "name": { "family": "Yakushin", "given": "I." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yoshida-S", "name": { "family": "Yoshida", "given": "S." } }, { "id": "Zawischa-I", "name": { "family": "Zawischa", "given": "I." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Analysis of LIGO data for gravitational waves from binary neutron stars", "ispublished": "pub", "full_text_status": "public", "keywords": "INSPIRALING COMPACT BINARIES; RELATIVISTIC GRAVITY; COALESCENCE RATES; SEARCH TEMPLATES; DETECTORS; PULSAR; INTERFEROMETER; SYSTEMS; FORMS; LASER", "note": "\u00a9 2004 The American Physical Society. \n\nReceived 6 October 2003; published 2 June 2004. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Ciencia y Tecnologia, the John Simon Guggenheim Foundation, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - ABBprd04d.pdf
", "abstract": "We report on a search for gravitational waves from coalescing compact binary systems in the Milky Way and the Magellanic Clouds. The analysis uses data taken by two of the three LIGO interferometers during the first LIGO science run and illustrates a method of setting upper limits on inspiral event rates using interferometer data. The analysis pipeline is described with particular attention to data selection and coincidence between the two interferometers. We establish an observational upper limit of R<1.7x10^(2) per year per Milky Way Equivalent Galaxy (MWEG), with 90% confidence, on the coalescence rate of binary systems in which each component has a mass in the range 1-3 M\u2609.", "date": "2004-06-15", "date_type": "published", "publication": "Physical Review D", "volume": "69", "number": "12", "publisher": "American Physical Society", "pagerange": "Art. No. 122001", "id_number": "CaltechAUTHORS:ABBprd04d", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd04d", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.69.122001", "primary_object": { "basename": "ABBprd04d.pdf", "url": "https://authors.library.caltech.edu/records/fyg3m-x4t84/files/ABBprd04d.pdf" }, "resource_type": "article", "pub_year": "2004", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/gxtzm-cd188", "eprint_id": 12967, "eprint_status": "archive", "datestamp": "2023-08-22 02:04:12", "lastmod": "2023-10-17 21:40:47", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Amin-R", "name": { "family": "Amin", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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E." } }, { "id": "Whiting-B-F", "name": { "family": "Whiting", "given": "B. F." }, "orcid": "0000-0002-8501-8669" }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Williams-P-R", "name": { "family": "Williams", "given": "P. R." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Willke-B", "name": { "family": "Willke", "given": "B." } }, { "id": "Wilson-A", "name": { "family": "Wilson", "given": "A." } }, { "id": "Winjum-B-J", "name": { "family": "Winjum", "given": "B. J." } }, { "id": "Winkler-W", "name": { "family": "Winkler", "given": "W." } }, { "id": "Wise-S", "name": { "family": "Wise", "given": "S." } }, { "id": "Wiseman-A-G", "name": { "family": "Wiseman", "given": "A. G." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Wooley-R", "name": { "family": "Wooley", "given": "R." } }, { "id": "Worden-J", "name": { "family": "Worden", "given": "J." } }, { "id": "Yakushin-I", "name": { "family": "Yakushin", "given": "I." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yoshida-S", "name": { "family": "Yoshida", "given": "S." } }, { "id": "Zawischa-I", "name": { "family": "Zawischa", "given": "I." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Analysis of first LIGO science data for stochastic gravitational waves", "ispublished": "pub", "full_text_status": "public", "keywords": "gravitational wave detectors; gravitational waves; light interferometry; stochastic processes", "note": "\u00a9 2004 American Physical Society. \n\nReceived 14 January 2004; published 30 June 2004. \n\nThe authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Ciencia y Tecnologia, the John Simon Guggenheim Foundation, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation. This paper has been assigned LIGO Document Number LIGO-P030009-H-Z.\n\nPublished - ABBprd04c.pdf
", "abstract": "We present the analysis of between 50 and 100 h of coincident interferometric strain data used to search for and establish an upper limit on a stochastic background of gravitational radiation. These data come from the first LIGO science run, during which all three LIGO interferometers were operated over a 2-week period spanning August and September of 2002. The method of cross correlating the outputs of two interferometers is used for analysis. We describe in detail practical signal processing issues that arise when working with real data, and we establish an observational upper limit on a f^-3 power spectrum of gravitational waves. Our 90% confidence limit is \u03a90h100(^2)<~23\u00b14.6 in the frequency band 40\u2013314 Hz, where h100 is the Hubble constant in units of 100 km/sec/Mpc and \u03a90 is the gravitational wave energy density per logarithmic frequency interval in units of the closure density. This limit is approximately 104 times better than the previous, broadband direct limit using interferometric detectors, and nearly 3 times better than the best narrow-band bar detector limit. As LIGO and other worldwide detectors improve in sensitivity and attain their design goals, the analysis procedures described here should lead to stochastic background sensitivity levels of astrophysical interest.", "date": "2004-06-15", "date_type": "published", "publication": "Physical Review D", "volume": "69", "number": "12", "publisher": "American Physical Society", "pagerange": "Art. No. 122004", "id_number": "CaltechAUTHORS:ABBprd04c", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd04c", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "John Simon Guggenheimn Foundation" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P030009-H-Z", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.69.122004", "primary_object": { "basename": "ABBprd04c.pdf", "url": "https://authors.library.caltech.edu/records/gxtzm-cd188/files/ABBprd04c.pdf" }, "resource_type": "article", "pub_year": "2004", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/5480n-w1p37", "eprint_id": 12810, "eprint_status": "archive", "datestamp": "2023-08-19 13:27:58", "lastmod": "2023-10-17 20:56:13", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Amin-R", "name": { "family": "Amin", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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G." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Wooley-R", "name": { "family": "Wooley", "given": "R." } }, { "id": "Worden-J", "name": { "family": "Worden", "given": "J." } }, { "id": "Yakushin-I", "name": { "family": "Yakushin", "given": "I." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yoshida-S", "name": { "family": "Yoshida", "given": "S." } }, { "id": "Zawischa-I", "name": { "family": "Zawischa", "given": "I." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } } ] }, "title": "First upper limits from LIGO on gravitational wave bursts", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2004 American Physical Society. \n\n(Received 7 January 2004; published 7 May 2004)\n\nThe authors gratefully acknowledge the support of the\nUnited States National Science Foundation for the construction\nand operation of the LIGO Laboratory and the Particle\nPhysics and Astronomy Research Council of the United\nKingdom, the Max-Planck-Society, and the State of\nNiedersachsen/Germany for support of the construction and\noperation of the GEO600 detector. The authors also gratefully\nacknowledge the support of the research by these agencies\nand by the Australian Research Council, the Natural\nSciences and Engineering Research Council of Canada, the\nCouncil of Scientific and Industrial Research of India, the\nDepartment of Science and Technology of India, the Spanish\nMinisterio de Ciencia y Tecnologia, the John Simon Guggenheim\nFoundation, the David and Lucile Packard Foundation,\nthe Research Corporation, and the Alfred P. Sloan Foundation.\nThis document has been assigned LIGO Laboratory\ndocument number LIGO-P030011.\n\nPublished - ABBprd04b.pdf
", "abstract": "We report on a search for gravitational wave bursts using data from the first science run of the Laser Interferometer Gravitational Wave Observatory (LIGO) detectors. Our search focuses on bursts with durations ranging from 4 to 100 ms, and with significant power in the LIGO sensitivity band of 150 to 3000 Hz. We bound the rate for such detected bursts at less than 1.6 events per day at a 90% confidence level. This result is interpreted in terms of the detection efficiency for ad hoc waveforms (Gaussians and sine Gaussians) as a function of their root-sum-square strain h(rss); typical sensitivities lie in the range h(rss) ~10^(-19)-10^(-17) strain/\u221aHz, depending on the waveform. We discuss improvements in the search method that will be applied to future science data from LIGO and other gravitational wave detectors.", "date": "2004-04-15", "date_type": "published", "publication": "Physical Review D", "volume": "69", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. No. 102001", "id_number": "CaltechAUTHORS:ABBprd04b", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd04b", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Council of Science and Industrial Research (India)" }, { "agency": "Ministerio de Ciencia Y Tecnologia (MCYT)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P030011", "name": "LIGO Laboratory" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "doi": "10.1103/PhysRevD.69.082004", "primary_object": { "basename": "ABBprd04b.pdf", "url": "https://authors.library.caltech.edu/records/5480n-w1p37/files/ABBprd04b.pdf" }, "resource_type": "article", "pub_year": "2004", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/eytb5-hty44", "eprint_id": 12781, "eprint_status": "archive", "datestamp": "2023-08-22 01:50:02", "lastmod": "2023-10-17 20:55:14", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Adhikari-R-X", "name": { "family": "Adhikari", "given": "Rana X." }, "orcid": "0000-0002-5731-5076" }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Amin-A", "name": { "family": "Amin", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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E." } }, { "id": "Whiting-B-F", "name": { "family": "Whiting", "given": "B. F." }, "orcid": "0000-0002-8501-8669" }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Williams-P-R", "name": { "family": "Williams", "given": "P. R." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Willke-B", "name": { "family": "Willke", "given": "B." } }, { "id": "Wilson-A", "name": { "family": "Wilson", "given": "A." } }, { "id": "Winjum-B-J", "name": { "family": "Winjum", "given": "B. J." } }, { "id": "Winkler-W", "name": { "family": "Winkler", "given": "W." } }, { "id": "Wise-S", "name": { "family": "Wise", "given": "S." } }, { "id": "Wiseman-A-G", "name": { "family": "Wiseman", "given": "A. G." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Wooley-R", "name": { "family": "Wooley", "given": "R." } }, { "id": "Worden-J", "name": { "family": "Worden", "given": "J." } }, { "id": "Yakushin-I", "name": { "family": "Yakushin", "given": "I." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Yoshida-S", "name": { "family": "Yoshida", "given": "S." } }, { "id": "Zawischa-I", "name": { "family": "Zawischa", "given": "I." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zotov-N", "name": { "family": "Zotov", "given": "N." } }, { "id": "Zucker-M-E", "name": { "family": "Zucker", "given": "M." }, "orcid": "0000-0002-2544-1596" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Setting upper limits on the strength of periodic gravitational waves from PSR J1939+2134 using the first science data from the GEO 600 and LIGO detectors", "ispublished": "pub", "full_text_status": "public", "keywords": "ROTATING RELATIVISTIC STARS; ACCRETING NEUTRON-STARS; X-RAY BINARIES; MILLISECOND PULSARS; RADIATION; INTERFEROMETER; INSTABILITY; B1937+21; SEARCH", "note": "\u00a9 2004 The American Physical Society. \n\nReceived 17 September 2003; published 30 April 2004. \n\nThe authors gratefully acknowledge the support of the U.S. National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max-Planck-Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research Council of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Ciencia y Tecnologia, the John Simon Guggenheim Foundation, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.\n\nPublished - ABBprd04a.pdf
", "abstract": "Data collected by the GEO 600 and LIGO interferometric gravitational wave detectors during their first observational science run were searched for continuous gravitational waves from the pulsar J1939+2134 at twice its rotation frequency. Two independent analysis methods were used and are demonstrated in this paper: a frequency domain method and a time domain method. Both achieve consistent null results, placing new upper limits on the strength of the pulsar's gravitational wave emission. A model emission mechanism is used to interpret the limits as a constraint on the pulsar's equatorial ellipticity.", "date": "2004-04-15", "date_type": "published", "publication": "Physical Review D", "volume": "69", "number": "8", "publisher": "American Physical Society", "pagerange": "Art. No. 082004", "id_number": "CaltechAUTHORS:ABBprd04a", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:ABBprd04a", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max Planck Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u00f3n y Ciencia (MEC)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1103/PhysRevD.69.082004", "primary_object": { "basename": "ABBprd04a.pdf", "url": "https://authors.library.caltech.edu/records/eytb5-hty44/files/ABBprd04a.pdf" }, "resource_type": "article", "pub_year": "2004", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/r1ztb-nt346", "eprint_id": 24344, "eprint_status": "archive", "datestamp": "2023-08-19 13:15:06", "lastmod": "2023-10-23 22:36:05", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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S." } }, { "id": "Tilav-S", "name": { "family": "Tilav", "given": "S." } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "M." }, "orcid": "0000-0002-8107-5148" }, { "id": "Torrie-C", "name": { "family": "Torrie", "given": "C." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ware-B", "name": { "family": "Ware", "given": "B." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" }, { "id": "Wilson-A", "name": { "family": "Wilson", "given": "A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "Alan J." }, "orcid": "0000-0002-0928-6784" } ] }, "title": "Upper limits on the strength of periodic gravitational waves from PSR J1939+2134", "ispublished": "pub", "full_text_status": "restricted", "note": "\u00a9 2004 IOP Publishing Ltd. Received 2 October 2003;\nPublished 9 February 2004. The authors gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Particle Physics and Astronomy Research Council of the United Kingdom, the Max\u2013Planck-Society and the State of Niedersachsen/Germany for support of the construction and operation of the GEO 600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Natural Sciences and Engineering Research\nCouncil of Canada, the Council of Scientific and Industrial Research of India, the Department of Science and Technology of India, the Spanish Ministerio de Ciencia y Tecnologia, the John Simon Guggenheim Foundation, the David and Lucile Packard Foundation, the Research Corporation and the Alfred P Sloan Foundation.", "abstract": "The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to test methods of searching for gravitational waves from known pulsars. Here we present new direct upper limits on the strength of waves from the pulsar PSR J1939+2134 using two independent analysis methods, one in the frequency domain using frequentist statistics and one in the time domain using Bayesian inference. Both methods show that the strain amplitude at Earth from this pulsar is less than a few times 10^(\u221222).", "date": "2004-03-07", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "21", "number": "5", "publisher": "IOP", "pagerange": "S671-S676", "id_number": "CaltechAUTHORS:20110708-115305907", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110708-115305907", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "Max-Planck-Society" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Educaci\u03ccn y Ciencia y Tecnologia" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" }, { "agency": "State of Niedersachsen/Germany" } ] }, "local_group": { "items": [ { "id": "TAPIR" }, { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1088/0264-9381/21/5/042", "resource_type": "article", "pub_year": "2004", "author_list": "Abbott, B.; Abbott, R.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/jsbsj-7ns42", "eprint_id": 49610, "eprint_status": "archive", "datestamp": "2023-08-22 01:38:23", "lastmod": "2023-10-17 21:34:50", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Allen-B", "name": { "family": "Allen", "given": "B." } }, { "id": "Woan-G", "name": { "family": "Woan", "given": "G." } }, { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Abbott-R", "name": { "family": "Abbott", "given": "R." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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T." } }, { "id": "Mageswaran-M", "name": { "family": "Mageswaran", "given": "M." } }, { "id": "Mailand-K", "name": { "family": "Mailand", "given": "K." } }, { "id": "Majid-W", "name": { "family": "Majid", "given": "W." } }, { "id": "Mann-F", "name": { "family": "Mann", "given": "F." } }, { "id": "M\u00e1rka-S", "name": { "family": "M\u00e1rka", "given": "S." } }, { "id": "Mason-J", "name": { "family": "Mason", "given": "J." } }, { "id": "Meshkov-S", "name": { "family": "Meshkov", "given": "S." } }, { "id": "Miyakawa-Osamu", "name": { "family": "Miyakawa", "given": "O." } }, { "id": "Miyoki-S", "name": { "family": "Miyoki", "given": "S." } }, { "id": "Mours-B", "name": { "family": "Mours", "given": "B." } }, { "id": "Nocera-F", "name": { "family": "Nocera", "given": "F." } }, { "id": "Ouimette-D", "name": { "family": "Ouimette", "given": "D." } }, { "id": "Pedraza-M", "name": { "family": "Pedraza", "given": "M." } }, { "id": "Rao-S-R", "name": { "family": "Rao", "given": "S. R." } }, { "id": "Redding-D", "name": { "family": "Redding", "given": "D." } }, { "id": "Regehr-M-W", "name": { "family": "Regehr", "given": "M. W." } }, { "id": "Reilly-K-T", "name": { "family": "Reilly", "given": "K. T." } }, { "id": "Reithmaier-K", "name": { "family": "Reithmaier", "given": "K." } }, { "id": "Robison-L", "name": { "family": "Robison", "given": "L." } }, { "id": "Romie-J", "name": { "family": "Romie", "given": "J." } }, { "id": "Rose-D", "name": { "family": "Rose", "given": "D." } }, { "id": "Russell-P", "name": { "family": "Russell", "given": "P." } }, { "id": "Salzman-I", "name": { "family": "Salzman", "given": "I." } }, { "id": "Sanders-G-H", "name": { "family": "Sanders", "given": "G. H." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Seel-S", "name": { "family": "Seel", "given": "S." } }, { "id": "Shawhan-P", "name": { "family": "Shawhan", "given": "P." } }, { "id": "Sievers-L", "name": { "family": "Sievers", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Spero-R", "name": { "family": "Spero", "given": "R." } }, { "id": "Sumner-M-C", "name": { "family": "Sumner", "given": "M. C." } }, { "id": "Sylvestre-J", "name": { "family": "Sylvestre", "given": "J." } }, { "id": "Takamori-A", "name": { "family": "Takamori", "given": "A." } }, { "id": "Tariq-H", "name": { "family": "Tariq", "given": "H." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Tilav-S", "name": { "family": "Tilav", "given": "S." } }, { "id": "Torrie-C", "name": { "family": "Torrie", "given": "C." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ware-B", "name": { "family": "Ware", "given": "B." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Wilson-A", "name": { "family": "Wilson", "given": "A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" } ] }, "title": "Upper limits on the strength of periodic gravitational waves from PSR J1939+2134", "ispublished": "pub", "full_text_status": "restricted", "keywords": "PACS: 04.80.Nn, 97.60.Gb, 95.75.Wx, 95.55.Ym, 95.75.Pq.\nMSC: 83C35 Gravitational waves, 85A35 Statistical astronomy.\nInstrumentation and measurement; Gravitation and cosmology; Astrophysics and astroparticles", "note": "\u00a9 2004 IOP Publishing Ltd.\nReceived 2 October 2003. Published 9 February 2004.\n\nThe authors gratefully acknowledge the support of the United States National Science\nFoundation for the construction and operation of the LIGO Laboratory and the Particle Physics\nand Astronomy Research Council of the United Kingdom, the Max\u2013Planck-Society and the\nState of Niedersachsen/Germany for support of the construction and operation of the GEO 600\ndetector. The authors also gratefully acknowledge the support of the research by these agencies\nand by the Australian Research Council, the Natural Sciences and Engineering Research\nCouncil of Canada, the Council of Scientific and Industrial Research of India, the Department\nof Science and Technology of India, the Spanish Ministerio de Ciencia y Tecnologia, the\nJohn Simon Guggenheim Foundation, the David and Lucile Packard Foundation, the Research\nCorporation and the Alfred P Sloan Foundation.", "abstract": "The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to test methods of searching for gravitational waves from known pulsars. Here we present new direct upper limits on the strength of waves from the pulsar PSR J1939+2134 using two independent analysis methods, one in the frequency domain using frequentist statistics and one in the time domain using Bayesian inference. Both methods show that the strain amplitude at Earth from this pulsar is less than a few times 10^(-22).", "date": "2004-03", "date_type": "published", "publication": "Classical and Quantum Gravity", "volume": "21", "number": "5, SI", "publisher": "IOP", "pagerange": "S671-S676", "id_number": "CaltechAUTHORS:20140911-121323448", "issn": "0264-9381", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140911-121323448", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Particle Physics and Astronomy Research Council (PPARC)" }, { "agency": "Max\u2013Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Ciencia y Tecnologia (MCYT)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1088/0264-9381/21/5/042", "resource_type": "article", "pub_year": "2004", "author_list": "Allen, B.; Woan, G.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/abqw9-48274", "eprint_id": 43290, "eprint_status": "archive", "datestamp": "2023-08-22 01:28:18", "lastmod": "2023-10-25 23:26:05", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Abbott-B-P", "name": { "family": "Abbott", "given": "B." } }, { "id": "Ageev-A", "name": { "family": "Ageev", "given": "A." } }, { "id": "Anderson-S-B", "name": { "family": "Anderson", "given": "S. 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H." } }, { "id": "Sannibale-V", "name": { "family": "Sannibale", "given": "V." } }, { "id": "Schmidt-V", "name": { "family": "Schmidt", "given": "V." } }, { "id": "Sears-B", "name": { "family": "Sears", "given": "B." } }, { "id": "Seel-S", "name": { "family": "Seel", "given": "S." } }, { "id": "Shawhan-P", "name": { "family": "Shawhan", "given": "P." } }, { "id": "Sievers-L", "name": { "family": "Sievers", "given": "L." } }, { "id": "Smith-M-R", "name": { "family": "Smith", "given": "M. R." } }, { "id": "Spero-R", "name": { "family": "Spero", "given": "R." } }, { "id": "Sumner-M-C", "name": { "family": "Sumner", "given": "M. C." } }, { "id": "Sylvestre-J", "name": { "family": "Sylvestre", "given": "J." } }, { "id": "Takamori-A", "name": { "family": "Takamori", "given": "A." } }, { "id": "Tariq-H", "name": { "family": "Tariq", "given": "H." } }, { "id": "Taylor-R", "name": { "family": "Taylor", "given": "R." } }, { "id": "Tilav-S", "name": { "family": "Tilav", "given": "S." } }, { "id": "Torrie-C", "name": { "family": "Torrie", "given": "C." } }, { "id": "Tyler-W", "name": { "family": "Tyler", "given": "W." } }, { "id": "Vass-S", "name": { "family": "Vass", "given": "S." } }, { "id": "Wallace-L", "name": { "family": "Wallace", "given": "L." } }, { "id": "Ware-B", "name": { "family": "Ware", "given": "B." } }, { "id": "Webber-D", "name": { "family": "Webber", "given": "D." } }, { "id": "Weinstein-Alan-J-Physics", "name": { "family": "Weinstein", "given": "A. J." }, "orcid": "0000-0002-0928-6784" }, { "id": "Wen-L", "name": { "family": "Wen", "given": "L." } }, { "id": "Whitcomb-S-E", "name": { "family": "Whitcomb", "given": "S. E." } }, { "id": "Willems-P-A", "name": { "family": "Willems", "given": "P. A." } }, { "id": "Wilson-A", "name": { "family": "Wilson", "given": "A." } }, { "id": "Yamamoto-Hiroaki", "name": { "family": "Yamamoto", "given": "H." } }, { "id": "Zhang-Liyuan", "name": { "family": "Zhang", "given": "L." }, "orcid": "0000-0002-0898-787X" }, { "id": "Zweizig-J", "name": { "family": "Zweizig", "given": "J." }, "orcid": "0000-0002-1521-3397" }, { "id": "Buonanno-A", "name": { "family": "Buonanno", "given": "A." } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Y." }, "orcid": "0000-0002-9730-9463" }, { "id": "Thorne-K-S", "name": { "family": "Thorne", "given": "K. S." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "M." }, "orcid": "0000-0002-4162-0033" }, { "id": "Drever-R-W-P", "name": { "family": "Drever", "given": "R. W. P." } }, { "id": "Tinto-M", "name": { "family": "Tinto", "given": "M." }, "orcid": "0000-0002-8107-5148" }, { "id": "Williams-R-D", "name": { "family": "Williams", "given": "R." }, "orcid": "0000-0002-9145-8580" } ] }, "title": "Detector description and performance for the first coincidence\n observations between LIGO and GEO", "ispublished": "pub", "full_text_status": "public", "keywords": "LIGO; Gravitational wave; Interferometer; Observatory", "note": "\u00a9 2003 Elsevier B.V. Received 30 September 2003. The authors gratefully acknowledge the support\nof the United States National Science Foundation\nfor the construction and operation of the LIGO\nLaboratory and the Particle Physics and Astronomy\nResearch Council of the United Kingdom,\nthe Max-Planck-Society and the State of Niedersachsen/\nGermany for support of the construction\nand operation of the GEO600 detector. The\nauthors also gratefully acknowledge the support\nof their research by these agencies and by the\nAustralian Research Council, the Natural Sciences\nand Engineering Research Council of Canada, the\nCouncil of Scientific and Industrial Research of\nIndia, the Department of Science and Technology\nof India, the Spanish Ministerio de Ciencia y\nTecnologia, the John Simon Guggenheim Foundation,\nthe David and Lucile Packard Foundation,\nthe Research Corporation, and the Alfred P. Sloan\nFoundation. This paper has been assigned LIGO\nLaboratory document number LIGO-P030024.\n\nSubmitted - 0308043v3.pdf
", "abstract": "For 17 days in August and September 2002, the LIGO and GEO interferometer gravitational wave detectors were operated in coincidence to produce their first data for scientific analysis. Although the detectors were still far from their design sensitivity levels, the data can be used to place better upper limits on the flux of gravitational waves incident on the earth than previous direct measurements. This paper describes the instruments and the data in some detail, as a companion to analysis papers based on the first data.", "date": "2004-01-21", "date_type": "published", "publication": "Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment", "volume": "517", "number": "1-3", "publisher": "Elsevier", "pagerange": "154-179", "id_number": "CaltechAUTHORS:20140109-094808747", "issn": "0168-9002", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140109-094808747", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF" }, { "agency": "Max-Planck-Society" }, { "agency": "State of Niedersachsen/Germany" }, { "agency": "Australian Research Council" }, { "agency": "Natural Sciences and Engineering Research Council of Canada (NSERC)" }, { "agency": "Council of Scientific and Industrial Research (India)" }, { "agency": "Department of Science and Technology (India)" }, { "agency": "Ministerio de Ciencia y Tecnologia (MCYT)" }, { "agency": "John Simon Guggenheim Foundation" }, { "agency": "David and Lucile Packard Foundation" }, { "agency": "Research Corporation" }, { "agency": "Alfred P. Sloan Foundation" } ] }, "other_numbering_system": { "items": [ { "id": "LIGO-P030024", "name": "LIGO Document" } ] }, "local_group": { "items": [ { "id": "LIGO" } ] }, "corp_creators": { "items": [ "LIGO Scientific Collaboration" ] }, "doi": "10.1016/j.nima.2003.11.124", "primary_object": { "basename": "0308043v3.pdf", "url": "https://authors.library.caltech.edu/records/abqw9-48274/files/0308043v3.pdf" }, "resource_type": "article", "pub_year": "2004", "author_list": "Abbott, B.; Ageev, A.; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/b1hev-n3017", "eprint_id": 49607, "eprint_status": "archive", "datestamp": "2023-08-19 11:27:06", "lastmod": "2023-10-23 15:42:21", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Buonanno-A", "name": { "family": "Buonanno", "given": "Alessandra" } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Yanbei" }, "orcid": "0000-0002-9730-9463" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit", "ispublished": "pub", "full_text_status": "public", "keywords": "PACS numbers: 04.30.Db, 04.25.Nx, 04.80.Nn, 95.55.Ym", "note": "Original: \u00a9 2003 The American Physical Society.\nReceived 27 November 2002. Published 30 May 2003.\n\nErratum: \u00a9 2006 The American Physical Society.\nReceived 11 July 2006. Published 31 July 2006.\nA small error in the computation of the gravitational wave flux in Refs. [1,2] propagates to the calculations of Ref. [3], and consequently to Eq. (1) of this paper.\n\nSpecial thanks go out to David Chernoff for having\nstarted the initial discussions and investigations that led to\nthis project. We thank Jolien Creighton, Thibault Damour,\nPhilippe Grandcle\u00b4ment, Vicky Kalogera, Yi Pan, Sterl Phinney,\nBangalore Sathyaprakash, and Kip Thorne for interesting\ndiscussions. We thank Thibault Damour for useful comments\non this manuscript and Cliff Will for clarifications on\nthe material discussed in Appendix A. We acknowledge support\nfrom NSF grant PHY-0099568 and NASA grant NAG5-10707. The research of A.B. was also supported by Caltech's\nRichard Chace Tolman Fund. The research of Y.C. was supported\nby the David and Barbara Groce Fund of the San\nDiego Foundation; the author thanks the gravitational-wave\ngroup at the Australian National University for their hospitality.\nPart of the research of M.V. was performed at the Jet\nPropulsion Laboratory, California Institute of Technology,\nunder contract with the National Aeronautics and Space Administration;\nthe author thanks the INFN group at the University\nof Parma, Italy, for their hospitality.\n\nErratum: Detecting gravitational waves from precessing binaries of spinning compact objects: Adiabatic limit [Phys. Rev. D 67, 104025 (2003)]\nAlessandra Buonanno, Yanbei Chen, and Michele Vallisneri\nPhys. Rev. D 74, 029904 (2006)\n\nPublished - PhysRevD.67.pdf
Erratum - PhysRevD.74.pdf
", "abstract": "Black-hole (BH) binaries with single-BH masses m=(5-20)M, moving on quasicircular orbits, are among the most promising sources for first-generation ground-based gravitational-wave (GW) detectors. Until now, the development of data-analysis techniques to detect GWs from these sources has been focused mostly on nonspinning BHs. The data-analysis problem for the spinning case is complicated by the necessity to model the precession-induced modulations of the GW signal, and by the large number of parameters needed to characterize the system, including the initial directions of the spins, and the position and orientation of the binary with respect to the GW detector. In this paper we consider binaries of maximally spinning BHs, and we work in the adiabatic-inspiral regime to build families of modulated detection templates that (i) are functions of very few physical and phenomenological parameters, (ii) model remarkably well the dynamical and precessional effects on the GW signal, with fitting factors on average greater than or similar to0.97, (iii) but, however, might require increasing the detection thresholds, offsetting at least partially the gains in the fitting factors. Our detection-template families are quite promising also for the case of neutron-star-black-hole binaries, with fitting factors on average approximate to0.93. For these binaries we also suggest (but do not test) a further template family, which would produce essentially exact waveforms written directly in terms of the physical spin parameters.", "date": "2003-05-15", "date_type": "published", "publication": "Physical Review D", "volume": "67", "number": "10", "publisher": "American Physical Society", "pagerange": "Art. 104025", "id_number": "CaltechAUTHORS:20140911-121322757", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140911-121322757", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "PHY-0099568" }, { "agency": "NASA", "grant_number": "NAG5-10707" }, { "agency": "Richard Chace Tolman Fund" }, { "agency": "David and Barbara Groce Fund of the San Diego Foundation" } ] }, "doi": "10.1103/PhysRevD.67.104025", "primary_object": { "basename": "PhysRevD.74.pdf", "url": "https://authors.library.caltech.edu/records/b1hev-n3017/files/PhysRevD.74.pdf" }, "related_objects": [ { "basename": "PhysRevD.67.pdf", "url": "https://authors.library.caltech.edu/records/b1hev-n3017/files/PhysRevD.67.pdf" } ], "resource_type": "article", "pub_year": "2003", "author_list": "Buonanno, Alessandra; Chen, Yanbei; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/zfx3k-wwq85", "eprint_id": 49605, "eprint_status": "archive", "datestamp": "2023-08-19 10:52:25", "lastmod": "2023-10-23 15:44:00", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Buonanno-A", "name": { "family": "Buonanno", "given": "Alessandra" } }, { "id": "Chen-Yanbei", "name": { "family": "Chen", "given": "Yanbei" }, "orcid": "0000-0002-9730-9463" }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Detection template families for gravitational waves from the final stages of binary-black-hole inspirals: Nonspinning case", "ispublished": "pub", "full_text_status": "public", "keywords": "PACS numbers: 04.30.Db, 04.25.Nx, 04.80.Nn, 95.55.Ym", "note": "\u00a9 2003 The American Physical Society.\nReceived 28 May 2002. Published 17 January 2003.\n\nWe wish to thank Kashif Alvi, Luc Blanchet, David Chernoff,\nTeviet Creighton, Thibault Damour, Scott Hughes, Albert\nLazzarini, Bangalore Sathyaprakash, Kip Thorne,\nMassimo Tinto and Andrea Vicere` for very useful discussions\nand interactions. We also thank Thibault Damour, Bangalore Sathyaprakash, and especially Kip Thorne for a very\ncareful reading of this manuscript and for stimulating comments;\nwe thank Luc Blanchet for useful discussions on the\nrelation between MECO and ISCO analyzed in Sec. IV A\nand David Chernoff for having shared with us his code for\nthe computation of the L model. We acknowledge support\nfrom NSF grant PHY-0099568. For A.B., this research was\nalso supported by Caltech's Richard Chase Tolman fund.\n\nErratum: Detection template families for gravitational waves from the final stages of binary\u2013black-hole inspirals: Nonspinning case [Phys. Rev. D 67, 024016 (2003)]\nAlessandra Buonanno, Yanbei Chen, and Michele Vallisneri\nPhys. Rev. D 74, 029903 (2006). http://dx.doi.org/10.1103/PhysRevD.74.029903\n\nPublished - PhysRevD.67.pdf
Erratum - PhysRevD.74.pdf
", "abstract": "We investigate the problem of detecting gravitational waves from binaries of nonspinning black holes with masses m=5-20M., moving on quasicircular orbits, which are arguably the most promising sources for first-generation ground-based detectors. We analyze and compare all the currently available post-Newtonian approximations for the relativistic two-body dynamics; for these binaries, different approximations predict different waveforms. We then construct examples of detection template families that embed all the approximate models and that could be used to detect the true gravitational-wave signal (but not to characterize accurately its physical parameters). We estimate that the fitting factor for our detection families is greater than or similar to0.95 (corresponding to an event rate loss less than or similar to15%) and we estimate that the discretization of the template family, for similar to10(4) templates, increases the loss to less than or similar to20%.", "date": "2003-01-17", "date_type": "published", "publication": "Physical Review D", "volume": "67", "number": "2", "publisher": "American Physical Society", "pagerange": "Art. 024016", "id_number": "CaltechAUTHORS:20140911-121322544", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140911-121322544", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "PHY-0099568" }, { "agency": "Richard C. Tolman Funds" } ] }, "doi": "10.1103/PhysRevD.67.024016", "primary_object": { "basename": "PhysRevD.67.pdf", "url": "https://authors.library.caltech.edu/records/zfx3k-wwq85/files/PhysRevD.67.pdf" }, "related_objects": [ { "basename": "PhysRevD.74.pdf", "url": "https://authors.library.caltech.edu/records/zfx3k-wwq85/files/PhysRevD.74.pdf" } ], "resource_type": "article", "pub_year": "2003", "author_list": "Buonanno, Alessandra; Chen, Yanbei; et el." }, { "id": "https://authors.library.caltech.eduhttps://authors.library.caltech.edu/records/nvdfq-pcq09", "eprint_id": 76242, "eprint_status": "archive", "datestamp": "2023-08-19 09:21:03", "lastmod": "2023-10-25 15:35:56", "type": "article", "metadata_visibility": "show", "creators": { "items": [ { "id": "Lindblom-L", "name": { "family": "Lindblom", "given": "Lee" } }, { "id": "Tohline-J-E", "name": { "family": "Tohline", "given": "Joel E." } }, { "id": "Vallisneri-M", "name": { "family": "Vallisneri", "given": "Michele" }, "orcid": "0000-0002-4162-0033" } ] }, "title": "Numerical evolutions of nonlinear r-modes in neutron stars", "ispublished": "pub", "full_text_status": "public", "note": "\u00a9 2002 American Physical Society. \n\n(Received 20 September 2001; published 9 April 2002) \n\nWe thank L. Bildsten, J. Friedman, Yu. Levin, B. Owen, N. Stergioulas, K. Thorne, G. Ushomirsky, and R. Wagoner for helpful discussions. We also thank H. Cohl, J. Cazes, and especially P. Motl for contributions to the LSU hydrodynamic code. This research was supported by NSF grants PHY-9796079, AST-9987344, AST-9731698, PHY-9900776, PHY-9907949, and PHY-0099568 and NASA grants NAG5-4093, NAG5-8497 and NAG5-10707. We thank NRAC for computing time on NPACI facilities at SDSC where tests were conducted; and we thank CACR for access to the HP V2500 computers at Caltech, where the primary simulations were performed.\n\nPublished - PhysRevD.65.084039.pdf
Accepted Version - 0109352.pdf
", "abstract": "Nonlinear evolution of the gravitational radiation (GR) driven instability in the r-modes of neutron stars is studied by full numerical 3D hydrodynamical simulations. The growth of the r-mode instability is found to be limited by the formation of shocks and breaking waves when the dimensionless amplitude of the mode grows to about three in value. This maximum mode amplitude is shown by numerical tests to be rather insensitive to the strength of the GR driving force. Upper limits on the strengths of possible nonlinear mode-mode coupling are inferred. Previously unpublished details of the numerical techniques used are presented, and the results of numerous calibration runs are discussed.", "date": "2002-04-15", "date_type": "published", "publication": "Physical Review D", "volume": "65", "number": "8", "publisher": "American Physical Society", "pagerange": "Art. No. 084039", "id_number": "CaltechAUTHORS:20170408-164428463", "issn": "2470-0010", "official_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170408-164428463", "rights": "No commercial reproduction, distribution, display or performance rights in this work are provided.", "funders": { "items": [ { "agency": "NSF", "grant_number": "PHY-9796079" }, { "agency": "NSF", "grant_number": "AST-9987344" }, { "agency": "NSF", "grant_number": "AST-9731698" }, { "agency": "NSF", "grant_number": "PHY-9900776" }, { "agency": "NSF", "grant_number": "PHY-9907949" }, { "agency": "NSF", "grant_number": "PHY-0099568" }, { "agency": "NASA", "grant_number": "NAG5-4093" }, { "agency": "NASA", "grant_number": "NAG5-8497" }, { "agency": "NASA", "grant_number": "NAG5-10707" } ] }, "local_group": { "items": [ { "id": "TAPIR" } ] }, "doi": "10.1103/PhysRevD.65.084039", "primary_object": { "basename": "0109352.pdf", "url": "https://authors.library.caltech.edu/records/nvdfq-pcq09/files/0109352.pdf" }, "related_objects": [ { "basename": "PhysRevD.65.084039.pdf", "url": "https://authors.library.caltech.edu/records/nvdfq-pcq09/files/PhysRevD.65.084039.pdf" } ], "resource_type": "article", "pub_year": "2002", "author_list": "Lindblom, Lee; Tohline, Joel E.; et el." } ]