XMM-Newton Proposal 03036701

Details XMM-Newton Proposal 03036701 XMM-Newton Proposal 03036701

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..133m&link_type=abstract

XMM-Newton Proposal ID #03036701

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rxj1419.3/Rxj14, Xmm-Newton Proposal 03036701

Scientific paper

A high-redshift double-cluster from the 160 Square Degree ROSAT survey provides an ideal laboratory for examining the formation and evolution of structure over a range of physical scales and evolutionary stages of the hierarchical clustering process. We have collected a wealth of optical data for these clusters and their surrounding environment. Principal components include a weak gravitational lensing analysis and deep, panoramic multi-color imaging of the galaxy populations, both of which were executed using the VLT 8m telescope. To complement these detailed assessments of the cold baryonic and dark matter components, and to measure the fundamental properties of the hot intracluster gas requires deep X-ray observations which we propose here.

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