Galaxy populations in massive galaxy clusters to z = 1.1: Colour distribution, concentration, halo occupation number and red sequence fraction

C. Hennig, J. J. Mohr, A. Zenteno, S. Desai, J. P. Dietrich, S. Bocquet, V. Strazzullo, A. Saro, T. M.C. Abbott, F. B. Abdalla, M. Bayliss, A. Benoit-Lévy, R. A. Bernstein, E. Bertin, D. Brooks, R. Capasso, D. Capozzi, A. Carnero, M. Carrasco Kind, J. CarreteroI. Chiu, C. B. D’Andrea, L. N. daCosta, H. T. Diehl, P. Doel, T. F. Eifler, A. E. Evrard, A. Fausti-Neto, P. Fosalba, J. Frieman, C. Gangkofner, A. Gonzalez, D. Gruen, R. A. Gruendl, N. Gupta, G. Gutierrez, K. Honscheid, J. Hlavacek-Larrondo, D. J. James, K. Kuehn, N. Kuropatkin, O. Lahav, M. March, J. L. Marshall, P. Martini, M. McDonald, P. Melchior, C. J. Miller, R. Miquel, E. Neilsen, B. Nord, R. Ogando, A. A. Plazas, C. Reichardt, A. K. Romer, E. Rozo, E. S. Rykoff, E. Sanchez, B. Santiago, M. Schubnell, I. Sevilla-Noarbe, R. C. Smith, M. Soares-Santos, F. Sobreira, B. Stalder, S. A. Stanford, E. Suchyta, M. E.C. Swanson, G. Tarle, D. Thomas, V. Vikram, A. R. Walker, Y. Zhang

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