Galaxy populations in massive galaxy clusters to z=1.1: colour distribution, concentration, halo occupation number and red sequence fraction
C Hennig, JJ Mohr, A Zenteno, S Desai, JP Dietrich, S Bocquet, V Strazzullo, A Saro, TMC Abbott, FB Abdalla, M Bayliss, A Benoit-Levy, RA Bernstein, E Bertin, D Brooks, R Capasso, D Capozzi, A Carnero, M Carrasco Kind, J Carretero Show all
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | OXFORD UNIV PRESS | Published : 2017
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Awarded by Transregio program
Awarded by Science and Technology Facilities Council
We acknowledge the support by the DFGCluster of Excellence `Origin and Structure of the Universe', the Transregio program TR33 `The Dark Universe' and the Ludwig-Maximilians-Universitat. The data processing has been carried out on the computing facilities of the Computational Center for Particle and Astrophysics (C2PAP), located at the Leibniz Supercomputer Center (LRZ).