(Spitzer Large
Area Survey with Hyper-Suprime-Cam)
https://splash.caltech.edu/
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the nature of bright z ≃ 7 galaxies with the Hubble Space Telescope;
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No change in global star formation process out to z > 3;
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Impossibly Early Galaxy Problem; Astrophysical Journal; Vol. 824;
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Absorption Lines as Metallicity Estimator: the Metal Content of
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galaxy UV luminosity function at z≃ 2–4; new results on faint-end slope
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Royal Astronomical Society; Vol. 456; No. 3; 3194-3211; 10.1093/mnras/stv2857
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SPLASH Survey: Quiescent Galaxies Are More Strongly Clustered but Are
Not Necessarily Located in High-density Environments; Astrophysical
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CHANDRA COSMOS Legacy Survey: Optical / IR Identifications;
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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
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Turnover in the Galaxy Main Sequence of Star Formation at M_* ~ 10^(10)
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Attenuation in High Redshift Galaxies: “Diamonds in the Sky”;
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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
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Splash Survey: A Spectroscopic Portrait of Andromeda’s Giant Southern
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