The representative XMM-Newton cluster structure survey (REXCESS) of an X-ray luminosity selected galaxy cluster sample
/ Authors
H. Boehringer, P. Schuecker, G. Pratt, M. Arnaud, T. Ponman, J. Croston, S. Borgani, R. Bower, U. Briel, C. Collins
and 24 more authors
M. Donahue, W. Forman, A. Finoguenov, M. Geller, L. Guzzo, J. Henry, R. Kneissl, J. Mohr, K. Matsushita, C. Mullis, T. Ohashi, K. Pedersen, D. Pierini, H. Quintana, Somak Raychaudhury, T. Reiprich, A. Romer, P. Rosati, K. Sabirli, R. Temple, P. Viana, A. Vikhlinin, G. Voit, Y.-Y. Zhang
/ Abstract
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.
Journal: Astronomy and Astrophysics