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III. Measuring the Stellar Velocity Dispersion Profile", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20180117-095337937", id = "record", issn = "1538-4357", doi = "10.3847/1538-4357/aa9f26", volume = "852", number = "2" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-104503624, title = "HST Imaging of the Brightest z \textasciitilde\ 8–9 Galaxies from UltraVISTA: The Extreme Bright End of the UV Luminosity Function", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-104503624", id = "record", issn = "1538-4357", doi = "10.3847/1538-4357/aa9a40", volume = "851", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-135713279, title = "G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR", journal = "Monthly Notices of the Royal Astronomical Society", publisher = "Oxford University Press", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-135713279", id = "record", issn = "0035-8711", doi = "10.1093/mnras/stw2395", volume = "464", number = "2" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-140248161, title = "The COSMOS2015 galaxy stellar mass function: Thirteen billion years of stellar mass assembly in ten snapshots", journal = "Astronomy and Astrophysics", publisher = "EDP Sciences", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-140248161", id = "record", issn = "0004-6361", doi = "10.1051/0004-6361/201730419", volume = "605" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-142531971, title = "The rest-frame optical (900nm) galaxy luminosity function at z \textasciitilde\ 4-7: abundance matching points to limited evolution in the M\_(STAR)/M\_(HALO) ratio at z ⩾ 4", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-142531971", id = "record", issn = "1538-4357", doi = "10.3847/1538-4357/aa72d8", volume = "843", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170625-172150566, title = "The SCUBA-2 Cosmology Legacy Survey: the nature of bright submm galaxies from 2 deg² of 850-μm imaging", journal = "Monthly Notices of the Royal Astronomical Society", publisher = "Monthly Notices of the Royal Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170625-172150566", id = "record", issn = "0035-8711", doi = "10.1093/mnras/stx861", volume = "469", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-105400473, title = "No evidence for Population III stars or a direct collapse black hole in the z = 6.6 Lyman α emitter 'CR7'", journal = "Monthly Notices of the Royal Astronomical Society", publisher = "Royal Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-105400473", id = "record", issn = "0035-8711", doi = "10.1093/mnras/stx839", volume = "469", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-131233779, title = "Unveiling the nature of bright z ≃ 7 galaxies with the Hubble Space Telescope", journal = "Monthly Notices of the Royal Astronomical Society", publisher = "Oxford University Press", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-131233779", id = "record", issn = "0035-8711", doi = "10.1093/mnras/stw3296", volume = "466", number = "3" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170626-150842064, title = "The nature of the Lyman α emitter CR7: a persisting puzzle", journal = "Monthly Notices of the Royal Astronomical Society: Letters", publisher = "Oxford University Press", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170626-150842064", id = "record", issn = "1745-3925", doi = "10.1093/mnrasl/slx029", volume = "468", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170310-104204574, title = "(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. IV. Physical properties derived from spectral energy distributions", journal = "Astronomy and Astrophysics", publisher = "EDP Sciences", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170310-104204574", id = "record", issn = "0004-6361", doi = "10.1051/0004-6361/201628128", volume = "597" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170310-101901398, title = "(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. III. Environments", journal = "Astronomy and Astrophysics", publisher = "EDP Sciences", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170310-101901398", id = "record", issn = "0004-6361", doi = "10.1051/0004-6361/201526989", volume = "597" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-134813790, title = "Characterizing the evolving K-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys", journal = "Monthly Notices of the Royal Astronomical Society", publisher = "Oxford University Press", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-134813790", id = "record", issn = "0035-8711", doi = "10.1093/mnras/stw2728", volume = "465", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-141332941, title = "Gas Fraction and depletion time of massive star-forming galaxies at z ∼ 3.2: No change in global star formation process out to z > 3", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-141332941", id = "record", issn = "0004-637X", doi = "10.3847/1538-4357/833/1/112", volume = "833", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20160707-104137561, title = "The Impossibly Early Galaxy Problem", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20160707-104137561", id = "record", issn = "0004-637X", doi = "10.3847/0004-637X/824/1/21", volume = "824", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-142851441, title = "z≳ 7 galaxies with red Spitzer/IRAC [3.6]-[4.5] colors in the full CANDELS data set: The brightest-known galaxies at z\textasciitilde\ 7-9 and a probable spectroscopic confirmation at z = 7.48", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-142851441", id = "record", issn = "0004-637X", doi = "10.3847/0004-637X/823/2/143", volume = "823", number = "2" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20160919-104756275, title = "The COSMOS2015 Catalog: Exploring the 1 < z < 6 Universe with Half a Million Galaxies", journal = "Astrophysical Journal Supplement Series", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20160919-104756275", id = "record", issn = "0067-0049", doi = "10.3847/0067-0049/224/2/24", volume = "224", number = "2" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20160623-120349827, title = "Rest-UV Absorption Lines as Metallicity Estimator: the Metal Content of Star-Forming Galaxies at z \textasciitilde\ 5", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20160623-120349827", id = "record", issn = "0004-637X", doi = "10.3847/0004-637X/822/1/29", volume = "822", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20160624-075417558, title = "A Coherent Study of Emission Lines from Broadband Photometry: Specific Star Formation Rates and [O III]/Hβ Ratio at 3 < z < 6", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20160624-075417558", id = "record", issn = "0004-637X", doi = "10.3847/0004-637X/821/2/122", volume = "821", number = "2" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-143424767, title = "The galaxy UV luminosity function at z≃ 2–4; new results on faint-end slope and the evolution of luminosity density", journal = "Monthly Notices of the Royal Astronomical Society", publisher = "Oxford University Press", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-143424767", id = "record", issn = "0035-8711", doi = "10.1093/mnras/stv2857", volume = "456", number = "3" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20160418-074725693, title = "The Chandra COSMOS Legacy survey: overview and point source catalog", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20160418-074725693", id = "record", issn = "0004-637X", doi = "10.3847/0004-637X/819/1/62", volume = "819", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20160303-154315200, title = "The SPLASH Survey: Quiescent Galaxies Are More Strongly Clustered but Are Not Necessarily Located in High-density Environments", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20160303-154315200", id = "record", issn = "0004-637X", doi = "10.3847/0004-637X/817/2/97", volume = "817", number = "2" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170628-144219700, title = "The CHANDRA COSMOS Legacy Survey: Optical / IR Identifications", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170628-144219700", id = "record", issn = "0004-637X", doi = "10.3847/0004-637X/817/1/34", volume = "817", number = "1" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20150714-105208366, title = "Evolution of the specific star formation rate function at z < 1.4 Dissecting the mass-SFR plane in COSMOS and GOODS", journal = "Astronomy and Astrophysics", publisher = "EDP Sciences", url = "https://resolver.caltech.edu/CaltechAUTHORS:20150714-105208366", id = "record", issn = "0004-6361", doi = "10.1051/0004-6361/201425176", volume = "579" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20170629-125450062, title = "The galaxy-halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS field", journal = "Monthly Notices of the Royal Astronomical Society", publisher = "Oxford University Press", url = "https://resolver.caltech.edu/CaltechAUTHORS:20170629-125450062", id = "record", issn = "0035-8711", doi = "10.1093/mnras/stv276", volume = "449", number = "2" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20150605-105722803, title = "(Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. I. Multiwavelength identifications and redshift distribution", journal = "Astronomy and Astrophysics", publisher = "EDP Sciences", url = "https://resolver.caltech.edu/CaltechAUTHORS:20150605-105722803", id = "record", issn = "0004-6361", doi = "10.1051/0004-6361/201425032", volume = "577" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20150416-115610730, title = "A Turnover in the Galaxy Main Sequence of Star Formation at M\_* \textasciitilde\ 10^(10) M\_☉ for Redshifts z < 1.3", journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20150416-115610730", id = "record", issn = "0004-637X", doi = "10.1088/0004-637X/801/2/80", volume = "801", number = "2" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20150323-145007978, title = {Dust Attenuation in High Redshift Galaxies: "Diamonds in the Sky"}, journal = "Astrophysical Journal", publisher = "American Astronomical Society", url = "https://resolver.caltech.edu/CaltechAUTHORS:20150323-145007978", id = "record", issn = "0004-637X", doi = "10.1088/0004-637X/800/2/108", volume = "800", number = "2" } @article{https://resolver.caltech.edu/CaltechAUTHORS:20141222-094115048, title = "Global Properties of M31's Stellar Halo from the SPLASH Survey. II. 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