[ { "id": "authors:8wgrr-qpq15", "collection": "authors", "collection_id": "8wgrr-qpq15", "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20190424-141803303", "type": "book_section", "title": "Fizeau interferometric imaging of Io volcanism with LBTI/LMIRcam", "book_title": "Optical and Infrared Interferometry IV", "author": [ { "family_name": "Leisenring", "given_name": "J. M.", "orcid": "0000-0002-0834-6140", "clpid": "Leisenring-J-M" }, { "family_name": "Hinz", "given_name": "P. M.", "orcid": "0000-0002-1954-4564", "clpid": "Hinz-P-M" }, { "family_name": "Skrutskie", "given_name": "M. F.", "clpid": "Skrutskie-M-F" }, { "family_name": "Skemer", "given_name": "A.", "orcid": "0000-0001-6098-3924", "clpid": "Skemer-A-J" }, { "family_name": "Woodward", "given_name": "C. E.", "clpid": "Woodward-C-E" }, { "family_name": "Veillet", "given_name": "C.", "clpid": "Veillet-C" }, { "family_name": "Arcidiacono", "given_name": "C.", "clpid": "Arcidiacono-C" }, { "family_name": "Bailey", "given_name": "V.", "orcid": "0000-0002-5407-2806", "clpid": "Bailey-V-P" }, { "family_name": "Bertero", "given_name": "M.", "clpid": "Bertero-M" }, { "family_name": "Boccacci", "given_name": "P.", "clpid": "Boccacci-P" }, { "family_name": "Conrad", "given_name": "A.", "orcid": "0000-0003-2872-0061", "clpid": "Conrad-A" }, { "family_name": "de Kleer", "given_name": "K.", "orcid": "0000-0002-9068-3428", "clpid": "de-Kleer-K-R" }, { "family_name": "de Pater", "given_name": "I.", "orcid": "0000-0002-4278-3168", "clpid": "de-Pater-I" }, { "family_name": "Defr\u00e8re", "given_name": "D.", "orcid": "0000-0003-3499-2506", "clpid": "Defr\u00e8re-D" }, { "family_name": "Hill", "given_name": "J.", "clpid": "Hill-J" }, { "family_name": "Hofmann", "given_name": "K.-H.", "clpid": "Hofmann-K-H" }, { "family_name": "Kaltenegger", "given_name": "L.", "clpid": "Kaltenegger-L" }, { "family_name": "La Camera", "given_name": "A.", "clpid": "La-Camera-A" }, { "family_name": "Nelson", "given_name": "M. J.", "clpid": "Nelson-M-J" }, { "family_name": "Schertl", "given_name": "D.", "clpid": "Schertl-D" }, { "family_name": "Spencer", "given_name": "J.", "clpid": "Spencer-J-R" }, { "family_name": "Weigelt", "given_name": "G.", "clpid": "Weigelt-G" }, { "family_name": "Wilson", "given_name": "J. C.", "clpid": "Wilson-J-C" } ], "contributor": [ { "family_name": "Rajagopal", "given_name": "Jayadev K.", "clpid": "Rajagopal-J-K" }, { "family_name": "Creech-Eakman", "given_name": "Michelle J.", "clpid": "Creech-Eakman-M-J" }, { "family_name": "Malbet", "given_name": "Fabien", "clpid": "Malbet-F" } ], "abstract": "The Large Binocular Telescope (LBT) houses two 8.4-meter mirrors separated by 14.4 meters on a common mount. Coherent combination of these two AO-corrected apertures via the LBT Interferometer (LBTI) produces Fizeau interferometric images with a spatial resolution equivalent to that of a 22.8-meter telescope and the light- gathering power of single 11.8-meter mirror. Capitalizing on these unique capabilities, we used LBTI/LMIRcam to image thermal radiation from volcanic activity on the surface of Io at M-Band (4.8 \u03bcm) over a range of parallactic angles. At the distance of Io, the M-Band resolution of the interferometric baseline corresponds to a physical distance of ~135 km, enabling high-resolution monitoring of Io volcanism such as ares and outbursts inaccessible from other ground-based telescopes operating in this wavelength regime. Two deconvolution routines are used to recover the full spatial resolution of the combined images, resolving at least sixteen known volcanic hot spots. Coupling these observations with advanced image reconstruction algorithms demonstrates the versatility of Fizeau interferometry and realizes the LBT as the first in a series of extremely large telescopes.", "doi": "10.1117/12.2057290", "isbn": "9780819496140", "publisher": "Society of Photo-optical Instrumentation Engineers (SPIE)", "place_of_publication": "Bellingham, WA", "publication_date": "2014-07-24", "pages": "Art. No. 91462S" }, { "id": "authors:dcbcq-g1n08", "collection": "authors", "collection_id": "dcbcq-g1n08", "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20190517-083445649", "type": "book_section", "title": "The performance of TripleSpec at Palomar", "book_title": "Ground-based and Airborne Instrumentation for Astronomy II", "author": [ { "family_name": "Herter", "given_name": "Terry L.", "orcid": "0000-0002-3856-8385", "clpid": "Herter-T-L" }, { "family_name": "Henderson", "given_name": "Charles P.", "clpid": "Henderson-C-P" }, { "family_name": "Wilson", "given_name": "John C.", "clpid": "Wilson-J-C" }, { "family_name": "Matthews", "given_name": "Keith Y.", "clpid": "Matthews-Keith-Astronomy" }, { "family_name": "Rahmer", "given_name": "Gustavo", "clpid": "Rahmer-G" }, { "family_name": "Bonati", "given_name": "Marco", "clpid": "Bonati-M" }, { "family_name": "Muirhead", "given_name": "Philip S.", "orcid": "0000-0002-0638-8822", "clpid": "Muirhead-P-S" }, { "family_name": "Adams", "given_name": "Joseph D.", "orcid": "0000-0001-7645-8913", "clpid": "Adams-J-D" }, { "family_name": "Lloyd", "given_name": "James P.", "clpid": "Lloyd-J-P" }, { "family_name": "Skrutskie", "given_name": "Michael F.", "clpid": "Skrutskie-M-F" }, { "family_name": "Moon", "given_name": "Dae-Sik", "orcid": "0000-0003-4200-5064", "clpid": "Moon-Dae-Sik" }, { "family_name": "Parshley", "given_name": "Stephen C.", "clpid": "Parshley-S-C" }, { "family_name": "Nelson", "given_name": "Matthew J.", "clpid": "Nelson-M-J" }, { "family_name": "Martinache", "given_name": "Frantz", "orcid": "0000-0003-1180-4138", "clpid": "Martinache-F" }, { "family_name": "Gull", "given_name": "George E.", "clpid": "Gull-G-E" } ], "contributor": [ { "family_name": "McLean", "given_name": "Ian S.", "clpid": "McLean-I-S" }, { "family_name": "Casali", "given_name": "Mark M.", "clpid": "Casali-M-M" } ], "abstract": "We report the performance of Triplespec from commissioning observations on the 200-inch Hale Telescope at Palomar Observatory. Triplespec is one of a set of three near-infrared, cross-dispersed spectrographs covering wavelengths from 1 - 2.4 microns simultaneously at a resolution of ~2700. At Palomar, Triplespec uses a 1\u00d730 arcsecond slit. Triplespec will be used for a variety of scientific observations, including moderate to high redshift galaxies, star formation, and low mass stars and brown dwarfs. When used in conjunction with an externally dispersed interferometer, Triplespec will also detect and characterize extrasolar planets.", "doi": "10.1117/12.789660", "isbn": "9780819472243", "publisher": "Society of Photo-Optical Instrumentation Engineers (SPIE)", "place_of_publication": "Bellingham, WA", "publication_date": "2008-07-09", "pages": "Art. No. 70140X" }, { "id": "authors:88y11-rk476", "collection": "authors", "collection_id": "88y11-rk476", "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180619-132039026", "type": "book_section", "title": "Mass producing an efficient NIR spectrograph", "author": [ { "family_name": "Wilson", "given_name": "J. C.", "clpid": "Wilson-J-C" }, { "family_name": "Henderson", "given_name": "Charles P.", "clpid": "Henderson-C-P" }, { "family_name": "Herter", "given_name": "Terry L.", "orcid": "0000-0002-3856-8385", "clpid": "Herter-T-L" }, { "family_name": "Matthews", "given_name": "K.", "clpid": "Matthews-Keith-Astronomy" }, { "family_name": "Skrutskie", "given_name": "M. F.", "clpid": "Skrutskie-M-F" }, { "family_name": "Adams", "given_name": "Joseph D.", "orcid": "0000-0001-7645-8913", "clpid": "Adams-J-D" }, { "family_name": "Moon", "given_name": "Dae-Sik", "orcid": "0000-0003-4200-5064", "clpid": "Moon-Dae-Sik" }, { "family_name": "Smith", "given_name": "Roger", "clpid": "Smith-R-M" }, { "family_name": "Gautier", "given_name": "Nick", "clpid": "Gautier-N" }, { "family_name": "Ressler", "given_name": "Mike", "clpid": "Ressler-M-E" }, { "family_name": "Soifer", "given_name": "B. T.", "orcid": "0000-0002-8112-1132", "clpid": "Soifer-B-T" }, { "family_name": "Lin", "given_name": "Sean", "clpid": "Lin-Sean" }, { "family_name": "Howard", "given_name": "J.", "clpid": "Howard-James" }, { "family_name": "LaMarr", "given_name": "J.", "clpid": "LaMarr-J" }, { "family_name": "Stolberg", "given_name": "T. M.", "clpid": "Stolberg-T-M" }, { "family_name": "Zink", "given_name": "J.", "clpid": "Zink-J-I" } ], "contributor": [ { "family_name": "Moorwood", "given_name": "Alan F. M.", "clpid": "Moorwood-A-F-M" }, { "family_name": "Iye", "given_name": "Masanori", "clpid": "Iye-Masanori" } ], "abstract": "Four institutions are collaborating to design and build three near identical \u03bb/\u0394\u03bb ~2700 cross-dispersed near-infrared spectrographs for use on various 5-10 meter telescopes. The instrument design addresses the common observatory need for efficient, reliable near-infrared spectrographs through such features as broad wavelength coverage across 6 simultaneous orders (0.8 - 2.4 \u00b5m) in echelle format, real-time slit viewing through separate optics and detector, and minimal moving parts. Lastly, the collaborators are saving money and increasing the likelihood of success through economies of scale and sharing intellectual capital.", "doi": "10.1117/12.550925", "publisher": "Society of Photo-optical Instrumentation Engineers (SPIE)", "publication_date": "2004-09-30" }, { "id": "authors:m1a15-0qd82", "collection": "authors", "collection_id": "m1a15-0qd82", "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20191107-093943394", "type": "book_section", "title": "Low-Luminosity Companions to Nearby Stars: Status of the 2MASS Data Search", "book_title": "Ultracool Dwarfs: New Spectral Types L and T", "author": [ { "family_name": "Kirkpatrick", "given_name": "J. D.", "orcid": "0000-0003-4269-260X", "clpid": "Kirkpatrick-J-D" }, { "family_name": "Gizis", "given_name": "J. E.", "orcid": "0000-0002-8916-1972", "clpid": "Gizis-J-E" }, { "family_name": "Burgasser", "given_name": "A. J.", "orcid": "0000-0002-6523-9536", "clpid": "Burgasser-A-J" }, { "family_name": "Wilson", "given_name": "J. C.", "clpid": "Wilson-J-C" }, { "family_name": "Dahn", "given_name": "C. C.", "clpid": "Dahn-C-C" }, { "family_name": "Monet", "given_name": "D. G.", "clpid": "Monet-D-G" }, { "family_name": "Reid", "given_name": "I. N.", "clpid": "Reid-I-N" }, { "family_name": "Liebert", "given_name": "J.", "clpid": "Liebert-J" } ], "contributor": [ { "family_name": "Jones", "given_name": "Hugh R. A.", "clpid": "Jones-H-R-A" }, { "family_name": "Steele", "given_name": "Iain A.", "clpid": "Steele-I-A" } ], "abstract": "We present 2MASS discoveries of four L and T dwarf companions to nearby stars. Using spectral types of the companions and age estimates of the primaries, we estimate masses for these discoveries and compare them to four other L and T dwarf companions from the literature. Temperatures range from ~2000 to ~750 K, ages range from ~0.2 to ~3 Gyr, and masses range from ~0.035 to ~0.075 MO.", "doi": "10.1007/978-3-642-56672-1_12", "isbn": "978-3-642-62682-1", "publisher": "Springer", "place_of_publication": "Berlin", "publication_date": "2001", "pages": "125-132" } ]