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Observing the buildaup of the colour-magnitude relation at redshift
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Observing the buildaup of the colour-magnitude relation at redshift
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Observing the buildaup of the colour-magnitude relation at redshift
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Journal Article
Observing the buildaup of the colour-magnitude relation at redshift
2004
Overview
We analyse the restaframe (U$-$V) colouramagnitude relation for 2 clusters at redshift 0.7 and 0.8, drawn from the ESO Distant Cluster Survey. By comparing them with the population of red galaxies in the Coma cluster, we show that the high redshift clusters exhibit a deficit of passive faint red galaxies. Our results show that the redasequence population cannot be explained in terms of a monolithic and synchronous formation scenario. A large fraction of faint passive galaxies in clusters today has moved onto the red sequence relatively recently as a consequence of the fact that their star formation activity has come to an end at $z<0.8$. To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html
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