Near-infrared luminosity function of galaxies in distant clusters

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The stellar mass function of

cluster galaxies at z~1.2

From the K-band LF it is possible to derive

an estimate of the stellar mass function:

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The LF bright end is already dominated by evolved galaxies morph. early types (Blakeslee et al. 2003) K* red-sequence gals early and late spectral types (Toft et al. 2004)

The stellar mass function of cluster galaxies at z~1.2 From the K-band LF it is possible to derive an estimate of the stellar mass function:

Page 1 and 2: Near-infrared luminosity function o
Page 3 and 4: Distant Galaxy Clusters We studied
Page 5 and 6: RDCS J1252+2927 @ z=1.24(Rosati et
Page 7 and 8: The Lynx supercluster 2 galaxy clus
Page 9 and 10: The K-band luminosity function at z
Page 11 and 12: The K-band luminosity function at z
Page 13: The K * redshift evolution up to re
Page 17 and 18: Massive galaxies with old stars i-z
Page 19: Conclusions - The evolution of the

Near-infrared luminosity function of galaxies in distant clusters

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