Physics
Scientific paper
Oct 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...72l&link_type=abstract
XMM-Newton Proposal ID #03021101
Physics
Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Sc1604+4320, Xmm-Newton Proposal 03021101
Scientific paper
We propose to obtain detailed X-ray data for an optically-selected supercluster at z = 0.9. This large scale structure contains at least seven massive clusters, most of which are known X-ray emitters. These observations will allow us to place accurate constraints on the temperature, surface-brightness profile, and mass fraction of the intracluster medium in the member clusters. The clusters are extremely well-studied in the optical; thus, the addition of XMM data will enable us to study the small-scale relation between the galaxies and gas, to quantify the variation between the X-ray/optical properties of clusters at a fixed epoch, and to explore a large scale system of clusters in the process of formation.
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