[ { "id": "authors:ah7h5-ktk07", "collection": "authors", "collection_id": "ah7h5-ktk07", "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20191127-100958634", "type": "book_section", "title": "Formation and Evolution of Planetary Systems: SIRTF Legacy Science in the VLT Era", "book_title": "The Origin of Stars and Planets: The VLT View", "author": [ { "family_name": "Meyer", "given_name": "M. R.", "orcid": "0000-0003-1227-3084", "clpid": "Meyer-M-R" }, { "family_name": "Backman", "given_name": "D.", "clpid": "Backman-D-E" }, { "family_name": "Beckwith", "given_name": "S. V. W.", "clpid": "Beckwith-S-V-W" }, { "family_name": "Brooke", "given_name": "T. Y.", "clpid": "Brooke-T-Y" }, { "family_name": "Carpenter", "given_name": "J. M.", "orcid": "0000-0003-2251-0602", "clpid": "Carpenter-J-M" }, { "family_name": "Cohen", "given_name": "M.", "orcid": "0000-0002-8033-5972", "clpid": "Cohen-M-H" }, { "family_name": "Gorti", "given_name": "U.", "clpid": "Gorti-U" }, { "family_name": "Henning", "given_name": "T.", "clpid": "Henning-Thomas" }, { "family_name": "Hillenbrand", "given_name": "L. A.", "clpid": "Hillenbrand-L-A" }, { "family_name": "Hines", "given_name": "D.", "orcid": "0000-0003-4653-6161", "clpid": "Hines-D-C" }, { "family_name": "Hollenbach", "given_name": "D.", "clpid": "Hollenbach-D-J" }, { "family_name": "Lunine", "given_name": "J.", "orcid": "0000-0003-2279-4131", "clpid": "Lunine-Jonathan-Irving" }, { "family_name": "Malhotra", "given_name": "R.", "orcid": "0000-0002-1226-3305", "clpid": "Malhotra-Renu" }, { "family_name": "Mamajek", "given_name": "E.", "orcid": "0000-0003-2008-1488", "clpid": "Mamajek-E-E" }, { "family_name": "Morris", "given_name": "P.", "orcid": "0000-0002-5186-4381", "clpid": "Morris-P-W" }, { "family_name": "Najita", "given_name": "J.", "clpid": "Najita-Joan-R" }, { "family_name": "Padgett", "given_name": "D. L.", "orcid": "0000-0001-5334-5107", "clpid": "Padgett-D-L" }, { "family_name": "Soderblom", "given_name": "D.", "orcid": "0000-0002-0322-8161", "clpid": "Soderblom-D-R" }, { "family_name": "Stauffer", "given_name": "J.", "orcid": "0000-0003-3595-7382", "clpid": "Stauffer-J-R" }, { "family_name": "Strom", "given_name": "S. E.", "clpid": "Strom-S-E" }, { "family_name": "Watson", "given_name": "D.", "clpid": "Watson-D" }, { "family_name": "Weidenschilling", "given_name": "S.", "clpid": "Weidenschilling-S" }, { "family_name": "Young", "given_name": "E.", "clpid": "Young-E-T" } ], "contributor": [ { "family_name": "Alves", "given_name": "Jo\u00e3o F.", "clpid": "Alves-J-F" }, { "family_name": "McCaughrean", "given_name": "Mark J.", "clpid": "McCaughrean-M-J" } ], "abstract": "We will utilize the sensitivity of SIRTF through the Legacy Science Program to carry out spectrophotometric observations of solar-type stars aimed at (1) defining the timescales over which terrestrial and gas giant planets are built, from measurements diagnostic of dust/gas masses and radial distributions; and (2) establishing the diversity of planetary architectures and the frequency of planetesimal collisions as a function of time through observations of circumstellar debris disks. Together, these observations will provide an astronomical context for understanding whether our solar system - and its habitable planet - is a common or a rare circumstance.\n\nAchieving our science goals requires measuring precise spectral energy distributions for a statistically robust sample capable of revealing evolutionary trends and the diversity of system outcomes. Our targets have been selected from two carefully assembled databases of solar-like stars: (1) a sample located within 50 pc of the Sun spanning an age range from 100-3000 Myr for which a rich set of ancillary measurements (e.g. metallicity, stellar activity, kinematics) are available; and (2) a selection located between 15 and 180 pc and spanning ages from 3 to 100 Myr. For stars at these distances SIRTF is capable of detecting stellar photospheres with SNR >30 at \u03bb\u226424\u03bc m for our entire sample, as well as achieving SNR >5 at the photospheric limit for over 50% of our sample at \u03bb=70\u03bc m. Thus we will provide a complete census of stars with excess emission down to the level produced by the dust in our present-day solar system.\n\nSIRTF observations obtained as part of this program will provide a rich Legacy for follow-up observations utilizing a variety of facilities including the VLT. More information concerning our program can be found at http://gould.as.arizona.edu/feps.", "doi": "10.1007/10856518_60", "isbn": "978-3-540-43541-9", "publisher": "Springer", "place_of_publication": "Berlin", "publication_date": "2003-10-15", "pages": "463-472" }, { "id": "authors:7gjgc-p5g68", "collection": "authors", "collection_id": "7gjgc-p5g68", "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170227-154325068", "type": "book_section", "title": "Photodissociation Regions in Young PN", "book_title": "Infrared Astronomy with Arrays: The Next Generation", "author": [ { "family_name": "Graham", "given_name": "James R.", "clpid": "Graham-J-R" }, { "family_name": "Herbst", "given_name": "T. M.", "clpid": "Herbst-T-M" }, { "family_name": "Beckwith", "given_name": "S.", "clpid": "Beckwith-S-V-W" }, { "family_name": "Matthews", "given_name": "K.", "clpid": "Matthews-K" }, { "family_name": "Neugebauer", "given_name": "G.", "clpid": "Neugebauer-G" }, { "family_name": "Serabyn", "given_name": "E.", "clpid": "Serabyn-E" }, { "family_name": "Soifer", "given_name": "B. T.", "orcid": "0000-0002-8112-1132", "clpid": "Soifer-B-T" } ], "contributor": [ { "family_name": "McLean", "given_name": "Ian S.", "clpid": "McLean-I-S" } ], "abstract": "Infrared imaging of H2 and PAH emission in NGG 7027 and BD+30 3639 reveals the presence of photodissociation regions in the neutral gas surrounding these young planetary nebulae.", "doi": "10.1007/978-94-011-1070-9_15", "isbn": "978-94-010-4466-0", "publisher": "Springer", "place_of_publication": "Dordrecht", "publication_date": "1994", "pages": "69-72" }, { "id": "authors:th7f6-qmp59", "collection": "authors", "collection_id": "th7f6-qmp59", "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20181121-090050084", "type": "book_section", "title": "Molecular Disks Around Young Stars", "book_title": "Structure and Dynamics of the Interstellar Medium", "author": [ { "family_name": "Sargent", "given_name": "Anneila I.", "orcid": "0000-0002-4633-5098", "clpid": "Sargent-A-I" }, { "family_name": "Beckwith", "given_name": "Steven V. W.", "clpid": "Beckwith-S-V-W" } ], "contributor": [ { "family_name": "Moles", "given_name": "Mariano", "clpid": "Moles-M" }, { "family_name": "Tenorio-Tagle", "given_name": "Guillermo", "clpid": "Tenorio-Tagle-G" }, { "family_name": "Melnick", "given_name": "Jorge", "clpid": "Melnick-J" } ], "abstract": "There is now a substantial body of evidence that disk-like structures of gas and dust surround many protostars and young stellar objects (e.g. Rodriguez, these proceedings). We are currently studying a number of these disks to establish whether they have properties compatible with those attributed to the proto-solar nebula, in the early stages of evolution of our solar system. The frequency with which such proto-planetary disks are associated with young stars is also being investigated.", "doi": "10.1017/S0252921100023769", "isbn": "9783540519560", "publisher": "Springer", "place_of_publication": "Berlin", "publication_date": "1989", "pages": "215-220" }, { "id": "authors:p0ppk-x0n26", "collection": "authors", "collection_id": "p0ppk-x0n26", "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200318-082248223", "type": "book_section", "title": "Moderate Resolution Spectroscopy For The Space Infrared Telescope Facility (SIRTF)", "book_title": "Cryogenic Optical Systems and Instruments II", "author": [ { "family_name": "Houck", "given_name": "J. R.", "clpid": "Houck-J-R" }, { "family_name": "Beckwith", "given_name": "S. V. W.", "clpid": "Beckwith-S-V-W" }, { "family_name": "Herter", "given_name": "T.", "orcid": "0000-0002-3856-8385", "clpid": "Herter-T-L" }, { "family_name": "Salpeter", "given_name": "E. E.", "clpid": "Salpeter-E-E" }, { "family_name": "Forrest", "given_name": "W. J.", "clpid": "Forrest-W-J" }, { "family_name": "Matthews", "given_name": "K.", "clpid": "Matthews-Keith-Astronomy" }, { "family_name": "Soifer", "given_name": "B. T.", "orcid": "0000-0002-8112-1132", "clpid": "Soifer-B-T" }, { "family_name": "Watson", "given_name": "D.", "clpid": "Watson-D" }, { "family_name": "Roellig", "given_name": "T.", "clpid": "Roellig-T-L" }, { "family_name": "Weedman", "given_name": "D.", "clpid": "Weedman-D-W" }, { "family_name": "Bauman", "given_name": "L. R.", "clpid": "Bauman-L-R" }, { "family_name": "Downey", "given_name": "C. H.", "clpid": "Downey-C-H" }, { "family_name": "Reitsema", "given_name": "H. J.", "clpid": "Reitsema-H-J" }, { "family_name": "Strecker", "given_name": "D. W.", "clpid": "Strecker-D-W" } ], "contributor": [ { "family_name": "Melugin", "given_name": "Ramsey K.", "clpid": "Melugin-R-K" } ], "abstract": "A conceptual design for an infrared spectrometer capable of both low resolution (\u03bb/\u0394-\u03bb = 50; 2.5-200 microns) and moderate resolution (1000; 4-200 microns) and moderate resolution (1000; 4-200 microns) has been developed. This facility instrument will permit the spectroscopic study in the infrared of objects ranging from within the solar system to distant galaxies. The spectroscopic capability provided by this instrument for SIRTF will give astronomers orders of magnitude greater sensitivity for the study of faint objects than had been previously available. The low resolution mode will enable detailed studies of the continuum radiation. The moderate resolution mode of the instrument will permit studies of a wide range of problems, from the infrared spectral signatures of small outer solar system bodies such as Pluto and the satellites of the giant planets, to investigations of more luminous active galaxies and QS0s at substantially greater distances. A simple design concept has been developed for the spectrometer which supports the science investigation with practical cryogenic engineering. Operational flexibility is preserved with a minimum number of mechanisms. The five modules share a common aperture, and all gratings share a single scan mechanism. High reliability is achieved through use of flight-proven hardware concepts and redundancy. The design controls the heat load into the SIRTF cryogen, with all heat sources other than the detectors operating at 7K and isolated from the 4K cold station. Two-dimensional area detector arrays are used in the 2.5-120\u03bcm bands to simultaneously monitor adjacent regions in extended objects and to measure the background near point sources.", "doi": "10.1117/12.966640", "isbn": "9780892526543", "publisher": "Society of Photo-Optical Instrumentation Engineers (SPIE)", "place_of_publication": "Bellingham, WA", "publication_date": "1986-07-18", "pages": "69-72" }, { "id": "authors:zzqdd-d7j94", "collection": "authors", "collection_id": "zzqdd-d7j94", "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200318-083716382", "type": "book_section", "title": "Moderate Resolution Spectroscopy For The Space Infrared Telescope Facility (SIRTF)", "book_title": "Instrumentation for Optical Remote Sensing from Space", "author": [ { "family_name": "Houck", "given_name": "J. R.", "clpid": "Houck-J-R" }, { "family_name": "Beckwith", "given_name": "S. V. W.", "clpid": "Beckwith-S-V-W" }, { "family_name": "Herter", "given_name": "T.", "orcid": "0000-0002-3856-8385", "clpid": "Herter-T-L" }, { "family_name": "Salpeter", "given_name": "E. E.", "clpid": "Salpeter-E-E" }, { "family_name": "Forrest", "given_name": "W. J.", "clpid": "Forrest-W-J" }, { "family_name": "Matthews", "given_name": "K.", "clpid": "Matthews-Keith-Astronomy" }, { "family_name": "Soifer", "given_name": "B. T.", "orcid": "0000-0002-8112-1132", "clpid": "Soifer-B-T" }, { "family_name": "Watson", "given_name": "D.", "clpid": "Watson-D" }, { "family_name": "Roellig", "given_name": "T.", "clpid": "Roellig-T-L" }, { "family_name": "Weedman", "given_name": "D.", "clpid": "Weedman-D-W" }, { "family_name": "Bauman", "given_name": "L. R.", "clpid": "Bauman-L-R" }, { "family_name": "Downey", "given_name": "C. H.", "clpid": "Downey-C-H" }, { "family_name": "Reitsema", "given_name": "H. J.", "clpid": "Reitsema-H-J" }, { "family_name": "Strecker", "given_name": "D. W.", "clpid": "Strecker-D-W" } ], "contributor": [ { "family_name": "Lear", "given_name": "John W.", "clpid": "Lear-J-W" }, { "family_name": "Monfils", "given_name": "Andre", "clpid": "Monfils-A" }, { "family_name": "Russak", "given_name": "Sidney L.", "clpid": "Russak-S-L" }, { "family_name": "Seeley", "given_name": "John S.", "clpid": "Seeley-J-S" } ], "abstract": "A conceptual design for an infrared spectrometer capable of both low resolution (\u03bb/\u0394-\u03bb = 50; 2.5-200 microns) and moderate resolution (1000; 4-200 microns) and moderate resolution (1000; 4-200 microns) has been developed. This facility instrument will permit the spectroscopic study in the infrared of objects ranging from within the solar system to distant galaxies. The spectroscopic capability provided by this instrument for SIRTF will give astronomers orders of magnitude greater sensitivity for the study of faint objects than had been previously available. The low resolution mode will enable detailed studies of the continuum radiation. The moderate resolution mode of the instrument will permit studies of a wide range of problems, from the infrared spectral signatures of small outer solar system bodies such as Pluto and the satellites of the giant planets, to investigations of more luminous active galaxies and QS0s at substantially greater distances. A simple design concept has been developed for the spectrometer which supports the science investigation with practical cryogenic engineering. Operational flexibility is preserved with a minimum number of mechanisms. The five modules share a common aperture, and all gratings share a single scan mechanism. High reliability is achieved through use of flight-proven hardware concepts and redundancy. The design controls the heat load into the SIRTF cryogen, with all heat sources other than the detectors operating at 7K and isolated from the 4K cold station. Two-dimensional area detector arrays are used in the 2.5-120\u03bcm bands to simultaneously monitor adjacent regions in extended objects and to measure the background near point sources.", "doi": "10.1117/12.951938", "isbn": "9780892526246", "publisher": "Society of Photo-Optical Instrumentation Engineers (SPIE)", "place_of_publication": "Bellingham, WA", "publication_date": "1986-05-01", "pages": "238-241" } ]