Galaxy Populations in the 26 most massive Galaxy Clusters in the South Pole Telescope SZE Survey
arXiv:1603.05981 · doi:10.1093/mnras/stw1649
Abstract
We present a study of the optical properties of the 26 most massive galaxy clusters selected within the SPT-SZ 2500 deg survey. This Sunyaev-Zel'dovich effect selected sample spans a redshift range of 0.10 < z < 1.13. We measure the galaxy radial profile, the luminosity function (LF), and the halo occupation number (HON) using optical data with a typical depth of + 2. The stacked radial profiles are consistent with a NFW profile with a concentration of for the red sequence (RS) and for the total population. Stacking the data in multiple redshift bins shows a hint of redshift evolution in the concentration when both the total population is used, and when only RS galaxies are used (at 2.1 and 2.8, respectively). The stacked LF shows a faint end slope for the total and for the RS population. The redshift evolution of is found to be consistent with a passively evolving Composite Stellar Population (CSP) model. By adopting the CSP model predictions, we explore the redshift evolution of the schechter parameters and . We find for the total population to be consistent with no evolution (0.3), while evidence of evolution for the red galaxies is mildly significant (1.1-2.1). The data show that the density /E(z) decreases with redshift, in tension with the self-similar expectation at a 2.4 level for the total population. The measured HON-mass relation has a lower normalization than previous studies at low redshift. Finally, our data support HON redshift evolution at a 2.1 level, with clusters at higher redshift containing fewer galaxies per unit mass to + 3 than their low-z counterparts [abridged].
arXiv comment14 pages, 7 figures, 2 tables, submitted to MNRAS, abstract abridged for arXiv submission
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