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20012009
most citedGalaxy-cluster gas-density distributions of the Representative XMM-Newton Cluster Structure Survey (REXCESS)

204 citations · 553 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.CO2009★ 136 cited

Substructure of the galaxy clusters in the REXCESS sample: observed statistics and comparison to numerical simulations

H. Boehringer, G. W. Pratt, M. Arnaud +6

We study the substructure statistics of a representative sample of galaxy clusters by means of two currently popular substructure characterisation methods, power ratios and centroi…

astro-ph2008★ 204 cited

Galaxy-cluster gas-density distributions of the Representative XMM-Newton Cluster Structure Survey (REXCESS)

J. H. Croston, G. W. Pratt, H. Boehringer +7

We present a study of the structural and scaling properties of the gas distributions in the intracluster medium (ICM) of 31 nearby (z < 0.2) clusters observed with XMM-Newton, whic…

astro-ph2005★ 103 cited

Structure and scaling of the entropy in nearby galaxy clusters

G. W. Pratt, M. Arnaud, E. Pointecouteau

Using XMM-Newton observations, we investigate the scaling and structural properties of the ICM entropy in a sample of 10 nearby (z < 0.2) relaxed galaxy clusters in the temperature…

astro-ph2001★ 66 cited

The X-ray surface brightness profiles of hot galaxy clusters up to z~0.8: evidence for self-similarity and constraints on Omega_0

M. Arnaud, N. Aghanim, D. M. Neumann

We study the ROSAT surface brightness profiles of a sample of 25 distant (0.3<z<0.83) hot (kT>3.5keV) clusters. For both open and flat cosmological models, the derived emission mea…

astro-ph2001★ 44 cited

Self-similarity of clusters of galaxies and the L_X-T relation

D. M. Neumann, M. Arnaud

In this paper based on ROSAT/PSPC data we investigate the emission measure profiles of a sample of hot clusters of galaxies (kT>3.5keV) in order to explain the differences between…