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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*
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.

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