Mass Constraints on High Redshift Clusters of Galaxies with XMM-Newton

Details Mass Constraints on High Redshift Clusters of Galaxies with XMM-Newton Mass Constraints on High Redshift Clusters of Galaxies with XMM-Newton

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..219h&link_type=abstract

XMM-Newton Proposal ID #04058601

Mathematics

Logic

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rcs 2327-0204, Xmm-Newton Proposal 04058601

Scientific paper

By virtue of their immense size, galaxy clusters can provide important constraints on cosmological parameters. Two elements are crucial to this effort: a large sample of clusters covering a wide range in redshift, and accurate mass determinations. The Red-sequence Cluster Survey (RCS) has discovered thousands of cluster candidates at 0.2

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