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

B. J. Maughan·L. R. Jones·H. Ebeling·C. Scharf
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Abstract

The X-ray properties of a sample of 11 high-redshift (0.6 1 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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B. J. Maughan, L. R. Jones, H. Ebeling, C. Scharf. 2005-10-14. The evolution of the cluster X-ray scaling relations in the WARPS sample at 0.6<z<1.0. https://doi.org/10.1111/j.1365-2966.2005.09717.x

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