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

2007249 citationsJournal Articlebronze Open Access

Authors

H. Böhringer · Max Planck Society

P. Schuecker · Max Planck Society

G. W. Pratt · Max Planck Society

M. Arnaud · CEA Paris-Saclay

T. J. Ponman · University of Birmingham

J. H. Croston · University of Hertfordshire

S. Borgani

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.

Topics & Keywords

Galaxies: Formation, Evolution, Phenomena Astrophysics and Cosmic Phenomena Astrophysical Phenomena and Observations

Publication Details

Published in: Astronomy and Astrophysics

Volume 469, Issue 1, pp. 363-377

DOI: 10.1051/0004-6361:20066740

Field-Weighted Citation Impact: 7.01

Command Palette

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

Authors

Abstract

Topics & Keywords

Publication Details