Katherine E. Whitaker, Mariska Kriek, Pieter G. van Dokkum, Rachel Bezanson, Gabriel Brammer, Marijn Franx, Ivo Labbe
We study the growth of the red sequence through the number density and
structural evolution of a sample of young and old quiescent galaxies at 01 that are almost
non-existent at z<1; their number density is 5 x 10^{-5} Mpc^{-3} at z=2,
whereas it is a factor of 10 less at z=0.5. The observed number densities of
young and old quiescent galaxies at z>1 are consistent with a simple model in
which all old quiescent galaxies were once identified as post-starburst
galaxies. We find that the overall population of quiescent galaxies have
smaller sizes and slightly more elongated shapes at higher redshift, in
agreement with other recent studies. Interestingly, the most recently quenched
galaxies at 1View original: http://arxiv.org/abs/1112.0313
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