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The Buildup of the Red Sequence in Galaxy Clusters sincez~ 0.8
2004
Astrophysical Journal
We study the rest-frame (U-V) color-magnitude relation in 4 clusters at redshifts 0.7-0.8, drawn from the ESO Distant Cluster Survey. We confirm that red-sequence galaxies in these clusters can be described as an old, passively-evolving population and we demonstrate, by comparison with the Coma cluster, that there has been significant evolution in the stellar mass distribution of red-sequence galaxies since z~0.75. The EDisCS clusters exhibit a deficiency of low luminosity passive red galaxies.
doi:10.1086/423373
fatcat:pow7i4glcvg4bnt3wdlruhjfb4