Near-infrared luminosity function of galaxies in distant clusters

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RDCS J1252+2927 @ z=1.24(Rosati et al. 2004)

T gas ~5.2keV,Mtot~1.6 . 10 14 M sun

Observed in Xrays (Chandra),optical

+ NIR (HST,VLT), IR (Spitzer)

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Mei et al (2005) RDCS J0910+5422 @ z=1.11(Stanford et al. 2002) T gas ~7keV,Mtot~5 . 10 14 M sun Observed in Xrays (Chandra), optical + NIR (HST,Palomar 0.85' 200”),IR ~ 400 (Spitzer) kpc @ z1.1

RDCS J1252+2927 @ z=1.24(Rosati et al. 2004) T gas ~5.2keV,Mtot~1.6 . 10 14 M sun Observed in Xrays (Chandra),optical + NIR (HST,VLT), IR (Spitzer)

Page 1 and 2: Near-infrared luminosity function o
Page 3: Distant Galaxy Clusters We studied
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 and 14: The K * redshift evolution up to re
Page 15 and 16: The stellar mass function of cluste
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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