The representative XMM-Newton cluster structure survey (REXCESS) of an X-ray luminosity selected galaxy cluster sample

Authors: H. Böhringer, P. Schuecker, G. W. Pratt, M. Arnaud, T. J. Ponman, J. H. Croston, S. Borgani, R. G. Bower, U. G. Briel, C. A. Collins, Megan Donahue, W. Forman, A. Finoguenov, Margaret J. Geller, L. Guzzo, J. P. Henry, R. Kneißl, J. J. Mohr, Kyoko Matsushita, C. R. Mullis, T. Ohashi, K. Pedersen, D. Pierini, H. Quintana, Somak Raychaudhury, T. H. Reiprich, A. K. Romer, P. Rosati, Kivanc Sabirli, R. F. Temple, P. T. P. Viana, A. Vikhlinin, G. Mark Voit, Y.-Y. Zhang - Astronomy and Astrophysics 2007 cited by 259

Context.The largest uncertainty for cosmological studies using clusters of galaxies is introduced by our limited knowledge of the statistics of galaxy cluster structure, and of the scaling relations between observables and cluster mass.