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Galaxy population study of the 26 most massive galaxy clusters within the SPT footprint

Published online by Cambridge University Press:  09 February 2015

Alfredo Zenteno
Alfredo Zenteno*
Affiliation:
Cerro Tololo Inter-American Observatory, Casilla 603, La Serena, Chile email: azenteno@ctio.noao.edu
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Abstract

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We present optical properties of the 26 most massive galaxy clusters in the South Pole Telescope 2500 sq-deg footprint. We find a general consistency between our results and results found in the literature on samples built with different selection techniques. Most interesting, we find a preference for an evolution in the slope of the Schechter function, α, with its value increasing at higher redshift.

Keywords

cluster of galaxies - galaxies: evolution - galaxies: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Issue S309: Galaxies in 3D across the Universe , July 2014 , pp. 355
Copyright
Copyright © International Astronomical Union 2015 

References

Bleem, L. E., Stalder, B., de Haan, T., et al. 2014, arXiv:1409.0850Google Scholar
Bruzual, G., Charlot, S., 2003, MNRAS, 344, 1000Google Scholar
Lin, Y.-T., Mohr, J. J., & Stanford, S. A. 2004, ApJ, 610, 745CrossRefGoogle Scholar
Williamson, R., Benson, B. A., High, F. W., et al. 2011, ApJ, 738, 139Google Scholar