4.7 Article

A deeper view of extremely red galaxies: the redshift distribution in the GOODS/CDFS ISAAC field

Journal

Publisher

OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2004.08044.x

Keywords

galaxies : evolution; galaxies : formation; galaxies : high-redshift

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We have analysed five-epoch Great Observatories Origins Deep Survey (GOODS) HST-ACS B, V, I-775 and z data sets (v. 1.0 release), in conjunction with existing VLT-ISAAC imaging in the J, H and K-s bands, to derive estimated redshifts for the sample of 198 extremely red galaxies (ERGs) with K-s < 22 (Vega) and (I-775-K-s) > 3.92 selected by Roche, Dunlop & Almaini (2003) from 50.4 arcmin(2) of the GOODS/Chandra Deep Field South. We find that, at this depth, the ERG population spans the redshift range 0.5 < z(phot) < 4.75 and over two decades in mass (similar to3 x 10(9) M-. to similar to3 x 10(11) M-.). Our results show that the dust-corrected red envelope of galaxy evolution is well modelled by a starburst at redshift z(f) = 5 followed thereafter by passive evolution. We explore the evolution of the ERG luminosity function (LF) from redshifts [z(phot)] = 1.0 to [z(phot)] = 2.5 and compare it with the global K-s-band LF at redshifts 1 < z(phot) < 2. We find that the bright end of the ERG LF does not decrease from redshifts [z(phot)] = 2.0 to [z(phot)] = 2.5 and we connect this fact with the presence of progenitors of the local L > L population at redshifts zphot > 2. We determine lower limits of c = (6.1 +/- 1.9) x 10(-5) Mpc(-3) and rho(c) = (2.1 +/- 1.1) x 10(-5) Mpc(-3) on the comoving densities of progenitors of local massive galaxies already assembled at redshifts zphot = 2.5 and zphot = 3.5, respectively. We have investigated the existence of high-redshift Lyman-break galaxies massive enough to be included in this ERG sample. Out of an initial list of 12 potential very high redshift candidates, we have identified two ERGs which have a high probability of lying at z(phot) > 4. We discuss the advantages of multicolour to single-colour selection techniques in obtaining reliable lists of very high redshift candidate sources, and present revised lower redshift estimates for sources previously claimed as potential z > 5 dropouts in recent studies.

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