XMM-Newton Proposal 03026105

Details XMM-Newton Proposal 03026105 XMM-Newton Proposal 03026105

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...97b&link_type=abstract

XMM-Newton Proposal ID #03026105

Mathematics

Logic

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rxcj0225-2928, Rxcj0616-4748, Rxcj1236-3354, Xmm-Newton Proposal 03026105

Scientific paper

To use clusters as sensitive probes to study the emergence of cosmic structure and to test cosmological models we need a better knowledge of the scaling relations of cluster mass and observable properties. To improve this situation a Large Program was approved in AO3 to study 34 well selected clusters in detail. Of the first obtained observations a relatively large fraction was spoiled by high background events. We demonstrate that our observational goals cannot be reached with these compromised observations and request the reobservation of 5 of the clusters with the largest loss of exposure time.

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