期刊
ASTROPHYSICAL JOURNAL
卷 699, 期 2, 页码 1333-1353出版社
IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/699/2/1333
关键词
cosmology: observations; galaxies: clusters: general; galaxies: evolution; galaxies: halos
资金
- Kavli Institute for Cosmological Physics (KICP)
- U.S. Department of Energy [DE-AC02-76SF00515]
- Stanford University
- Alfred P. Sloan Foundation
- Participating Institutions
- National Science Foundation
- U.S. Department of Energy
- National Aeronautics and Space Administration
- Japanese Monbukagakusho
- Max Planck Society
- Higher Education Funding Council for England
Imaging data from the Sloan Digital Sky Survey are used to characterize the population of galaxies in groups and clusters detected with the MaxBCG algorithm. We investigate the dependence of brightest cluster galaxy (BCG) luminosity, and the distributions of satellite galaxy luminosity and satellite color, on cluster properties over the redshift range 0.1 <= z <= 0.3. The size of the data set allows us to make measurements in many bins of cluster richness, radius and redshift. We find that, within r(200) of clusters with mass above 3 x 10(13) h(-1) M-circle dot, the luminosity function (LF) of both red and blue satellites is only weakly dependent on richness. We further find that the shape of the satellite LF does not depend on cluster-centric distance for magnitudes brighter than M-0.25(i) - 5log(10)h = - 19. However, the mix of faint red and blue galaxies changes dramatically. The satellite red fraction is dependent on cluster-centric distance, galaxy luminosity, and cluster mass, and also increases by similar to 5% between redshifts 0.28 and 0.2, independent of richness. We find that BCG luminosity is tightly correlated with cluster richness, scaling as L-BCG similar to M-200(0.3), and has a Gaussian distribution at fixed richness, with sigma(logL) similar to 0.17 for massive clusters. The ratios of BCG luminosity to total cluster luminosity and characteristic satellite luminosity scale strongly with cluster richness: in richer systems, BCGs contribute a smaller fraction of the total light, but are brighter compared to typical satellites. This study demonstrates the power of cross-correlation techniques for measuring galaxy populations in purely photometric data.
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