XMM-Newton Proposal 02013303

Details XMM-Newton Proposal 02013303 XMM-Newton Proposal 02013303

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop...73z&link_type=abstract

XMM-Newton Proposal ID #02013303

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Cl1040-1155, Cl1054-1146, Cl1054-1245, Xmm-Newton Proposal 02013303

Scientific paper

We propose to compare X-ray luminosities and temperatures of a sample of confirmed optically-selected z~0.7 clusters to well-determined velocity dispersions and weak-lensing maps. The use of non-X-ray selected clusters enables us to search for large deviations in the X-ray properties relative to other mass tracers. Our extensive VLT, HST, and NTT observational program has provided velocity measurements for between 30 and 60 cluster members per cluster and weak lensing maps augmented with photometric redshift information for six of the most optically luminous clusters at z ~ 0.7 in the Las Campanas Distant Cluster Survey. Here we propose to continue this study by observing three more of these clusters.

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