The X-ray temperature function and structure of clusters at z=0.6-1

Details The X-ray temperature function and structure of clusters at z=0.6-1 The X-ray temperature function and structure of clusters at z=0.6-1

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..113m&link_type=abstract

XMM-Newton Proposal ID #05029502

Mathematics

Logic

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Cl2038.4-0125, Cl0035.9+8513, Xmm-Newton Proposal 05029502

Scientific paper

Under very general theoretical assumptions, the evolution of the space density of clusters of galaxies is extremely sensitive to cosmological parameters. The most straightforward method of exploiting this sensitivity is through measurements of the X-ray temperature function. We propose to reobserve two clusters that were awarded time in previous XMM AOs but whose data were rendered unusable due to high background periods. These clusters are required to finish the statistically complete sample needed to measure the temperature function.

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