Conditional quenching: a detailed look at the SFR−density relation at $z$ ∼ 0.9 from ORELSE

Abstract We present a study of the star formation rate (SFR)–density relation at $z$ ∼ 0.9 using data drawn from the Observations of Redshift Evolution in Large Scale Environments (ORELSE) survey. We find that SFR does depend on environment, but only for intermediate-stellar mass galaxies (1010.1 &l...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2019-04, Vol.484 (4), p.4695-4710
Hauptverfasser: Tomczak, Adam R, Lemaux, Brian C, Lubin, Lori M, Pelliccia, Debora, Shen, Lu, Gal, Roy R, Hung, Denise, Kocevski, Dale D, Le Fèvre, Olivier, Mei, Simona, Rumbaugh, Nicholas, Squires, Gordon K, Wu, Po-Feng
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Sprache:eng
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