The evolution of the cluster X-ray scaling relations in the WARPS sample at 0.6<z<1.0

Details The evolution of the cluster X-ray scaling relations in the WARPS sample at 0.6<z<1.0 The evolution of the cluster X-ray scaling relations in the WARPS sample at 0.6<z<1.0

2005-03-21

arxiv.org/abs/astro-ph/0503455v2

Mon.Not.Roy.Astron.Soc. 365 (2006) 509-529

Astronomy and Astrophysics

Astrophysics

23 pages, 17 figures. Accepted for publication in MNRAS. Revised to match accepted version: reanalysed data with latest calibr

Scientific paper

10.1111/j.1365-2966.2005.09717.x

The X-ray properties of a sample of 11 high-redshift (0.61 or in the early stages of the clusters' formation, prior to their observation. The properties of the intra-cluster medium at high-redshift are found to be similar to those in the local universe. The mean surface-brightness profile slope for the sample is 0.66+/-0.05, the mean gas mass fractions within R2500 and R200 are 0.073+/-0.010 and 0.12+/-0.02 respectively, and the mean metallicity of the sample is 0.28+/-0.16 solar.

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