SPLASH

(Spitzer Large Area Survey with Hyper-Suprime-Cam)

Articles from CaltechAUTHORS

• Hatfield, P. W.; Bowler, R. A. A.; et al. (2018) The environment and host haloes of the brightest z ~ 6 Lyman-break galaxies; Monthly Notices of the Royal Astronomical Society; Vol. 477; No. 3; 3760-3774; 10.1093/mnras/sty856
• Mehta, Vihang; Scarlata, Claudia; et al. (2018) SPLASH-SXDF Multi-wavelength Photometric Catalog; Astrophysical Journal Supplement Series; Vol. 235; No. 2; Art. No. 36; 10.3847/1538-4365/aab60c
• Gilbert, Karoline M.; Tollerud, Erik J.; et al. (2018) Global Properties of M31’s Stellar Halo from the SPLASH Survey. III. Measuring the Stellar Velocity Dispersion Profile; Astrophysical Journal; Vol. 852; No. 2; Art. No. 128; 10.3847/1538-4357/aa9f26
• Stefanon, Mauro; Labbé, Ivo; et al. (2017) HST Imaging of the Brightest z ~ 8–9 Galaxies from UltraVISTA: The Extreme Bright End of the UV Luminosity Function; Astrophysical Journal; Vol. 851; No. 1; Art. No. 43; 10.3847/1538-4357/aa9a40
• Andrews, S. K.; Driver, S. P.; et al. (2017) G10/COSMOS: 38 band (far-UV to far-IR) panchromatic photometry using LAMBDAR; Monthly Notices of the Royal Astronomical Society; Vol. 464; No. 2; 1569-1590; 10.1093/mnras/stw2395
• Davidzon, I.; Ilbert, O.; et al. (2017) The COSMOS2015 galaxy stellar mass function: Thirteen billion years of stellar mass assembly in ten snapshots; Astronomy and Astrophysics; Vol. 605; Art. No. A70; 10.1051/0004-6361/201730419
• Stefanon, Mauro; Bouwens, Rychard J.; et al. (2017) The rest-frame optical (900nm) galaxy luminosity function at z ~ 4-7: abundance matching points to limited evolution in the M_(STAR)/M_(HALO) ratio at z ⩾ 4; Astrophysical Journal; Vol. 843; No. 1; Art. No. 36; 10.3847/1538-4357/aa72d8
• Michałowski, Michał J.; Dunlop, J. S.; et al. (2017) The SCUBA-2 Cosmology Legacy Survey: the nature of bright submm galaxies from 2 deg² of 850-μm imaging; Monthly Notices of the Royal Astronomical Society; Vol. 469; No. 1; 492-515; 10.1093/mnras/stx861
• Bowler, R. A. A.; McLure, R. J.; et al. (2017) No evidence for Population III stars or a direct collapse black hole in the z = 6.6 Lyman α emitter ‘CR7’; Monthly Notices of the Royal Astronomical Society; Vol. 469; No. 1; 448-458; 10.1093/mnras/stx839
• Bowler, R. A. A.; Dunlop, J. S.; et al. (2017) Unveiling the nature of bright z ≃ 7 galaxies with the Hubble Space Telescope; Monthly Notices of the Royal Astronomical Society; Vol. 466; No. 3; 3612-3635; 10.1093/mnras/stw3296
• Pacucci, Fabio; Pallottini, Andrea; et al. (2017) The nature of the Lyman α emitter CR7: a persisting puzzle; Monthly Notices of the Royal Astronomical Society: Letters; Vol. 468; No. 1; L77-L81; 10.1093/mnrasl/slx029
• Miettinen, O.; Delvecchio, I.; et al. (2017) (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. IV. Physical properties derived from spectral energy distributions; Astronomy and Astrophysics; Vol. 597; Art. No. A5; 10.1051/0004-6361/201628128
• Smolčić, V.; Miettinen, O.; et al. (2017) (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. III. Environments; Astronomy and Astrophysics; Vol. 597; Art. No. A4; 10.1051/0004-6361/201526989
• Mortlock, Alice; McLure, Ross J.; et al. (2017) Characterizing the evolving K-band luminosity function using the UltraVISTA, CANDELS and HUDF surveys; Monthly Notices of the Royal Astronomical Society; Vol. 465; No. 1; 672-687; 10.1093/mnras/stw2728
• Schinnerer, E.; Groves, B.; et al. (2016) 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; Astrophysical Journal; Vol. 833; No. 1; Art No 112; 10.3847/1538-4357/833/1/112
• Steinhardt, Charles. L.; Capak, Peter; et al. (2016) The Impossibly Early Galaxy Problem; Astrophysical Journal; Vol. 824; No. 1; Art. No. 21; 10.3847/0004-637X/824/1/21
• Roberts-Borsani, G. W.; Bouwens, R. J.; et al. (2016) z≳ 7 galaxies with red Spitzer/IRAC [3.6]-[4.5] colors in the full CANDELS data set: The brightest-known galaxies at z~ 7-9 and a probable spectroscopic confirmation at z = 7.48; Astrophysical Journal; Vol. 823; No. 2; Art. No. 143; 10.3847/0004-637X/823/2/143
• Laigle, C.; Capak, P.; et al. (2016) The COSMOS2015 Catalog: Exploring the 1 < z < 6 Universe with Half a Million Galaxies; Astrophysical Journal Supplement Series; Vol. 224; No. 2; Art. No. 24; 10.3847/0067-0049/224/2/24
• Faisst, A. L.; Capak, P. L.; et al. (2016) Rest-UV Absorption Lines as Metallicity Estimator: the Metal Content of Star-Forming Galaxies at z ~ 5; Astrophysical Journal; Vol. 822; No. 1; Art. No. 29; 10.3847/0004-637X/822/1/29
• Faisst, A. L.; Capak, P.; et al. (2016) A Coherent Study of Emission Lines from Broadband Photometry: Specific Star Formation Rates and [O III]/Hβ Ratio at 3 < z < 6; Astrophysical Journal; Vol. 821; No. 2; Art. No. 122; 10.3847/0004-637X/821/2/122
• Civano, F.; Capak, P.; et al. (2016) The Chandra COSMOS Legacy survey: overview and point source catalog; Astrophysical Journal; Vol. 819; No. 1; Art. No. 62; 10.3847/0004-637X/819/1/62
• Parsa, Shaghayegh; Dunlop, James S.; et al. (2016) The galaxy UV luminosity function at z≃ 2–4; new results on faint-end slope and the evolution of luminosity density; Monthly Notices of the Royal Astronomical Society; Vol. 456; No. 3; 3194-3211; 10.1093/mnras/stv2857
• Lin, Lihwai; Capak, P. L.; et al. (2016) The SPLASH Survey: Quiescent Galaxies Are More Strongly Clustered but Are Not Necessarily Located in High-density Environments; Astrophysical Journal; Vol. 817; No. 2; Art. No. 97; 10.3847/0004-637X/817/2/97
• Marchesi, S.; Civano, F.; et al. (2016) The CHANDRA COSMOS Legacy Survey: Optical / IR Identifications; Astrophysical Journal; Vol. 817; No. 1; Art No 34; 10.3847/0004-637X/817/1/34
• Ilbert, O.; Arnouts, S.; et al. (2015) Evolution of the specific star formation rate function at z < 1.4 Dissecting the mass-SFR plane in COSMOS and GOODS; Astronomy and Astrophysics; Vol. 579; Art. No. A2; 10.1051/0004-6361/201425176
• Coupon, J.; Arnouts, S.; et al. (2015) The galaxy-halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS field; Monthly Notices of the Royal Astronomical Society; Vol. 449; No. 2; 1352-1379; 10.1093/mnras/stv276
• Miettinen, O.; Smolčić, V.; et al. (2015) (Sub)millimetre interferometric imaging of a sample of COSMOS/AzTEC submillimetre galaxies. I. Multiwavelength identifications and redshift distribution; Astronomy and Astrophysics; Vol. 577; Art. No. A29; 10.1051/0004-6361/201425032
• Lee, Nicholas; Sanders, D. B.; et al. (2015) A Turnover in the Galaxy Main Sequence of Star Formation at M_* ~ 10^(10) M_☉ for Redshifts z < 1.3; Astrophysical Journal; Vol. 801; No. 2; Art. No. 80; 10.1088/0004-637X/801/2/80
• Scoville, Nick; Faisst, Andreas; et al. (2015) Dust Attenuation in High Redshift Galaxies: “Diamonds in the Sky”; Astrophysical Journal; Vol. 800; No. 2; Art. No. 108; 10.1088/0004-637X/800/2/108
• Gilbert, Karoline M.; Kalirai, Jason S.; et al. (2014) Global Properties of M31’s Stellar Halo from the SPLASH Survey. II. Metallicity Profile; Astrophysical Journal; Vol. 796; No. 2; Art. No. 76; 10.1088/0004-637X/796/2/76
• Steinhardt, Charles L.; Speagle, Josh S.; et al. (2014) Star Formation at 4 < z < 6 from the Spitzer Large Area Survey with Hyper-Suprime-Cam (SPLASH); Astrophysical Journal Letters; Vol. 791; No. 2; Art. No. L25; 10.1088/2041-8205/791/2/L25
• Bowler, R. A. A.; Dunlop, J. S.; et al. (2014) The bright end of the galaxy luminosity function at z =7: before the onset of mass quenching?; Monthly Notices of the Royal Astronomical Society; Vol. 440; No. 3; 2810-2842; 10.1093/mnras/stu449
• Kalirai, Jason S.; Beaton, Rachael L.; et al. (2010) The SPLASH Survey: Internal Kinematics, Chemical Abundances, and Masses of the Andromeda I, II, III, VII, X, and XIV Dwarf Spheroidal Galaxies; Astrophysical Journal; Vol. 711; No. 2; 671-692; 10.1088/0004-637X/711/2/671
• Gilbert, Karoline M.; Guhathakurta, Puragra; et al. (2009) The Splash Survey: A Spectroscopic Portrait of Andromeda’s Giant Southern Stream; Astrophysical Journal; Vol. 705; No. 2; 1275-1297; 10.1088/0004-637X/705/2/1275