Cosmology and Astrophysics with the Most Massive Intermediate redshift Clusters

Details Cosmology and Astrophysics with the Most Massive Intermediate redshift Clusters Cosmology and Astrophysics with the Most Massive Intermediate redshift Clusters

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop...85c&link_type=abstract

XMM-Newton Proposal ID #06720905

Mathematics

Logic

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rxcj0013.2-4905, Rxcj0018.9-4051, Rxcj0217.2-5244, Rxcj0243.6-4834

Scientific paper

The most X-ray luminous and massive galaxy clusters are the most interesting objects for astrophysical and cosmological studies. Completing our REFELX 2 cluster survey, we can now add another 10 of the most luminous clusters in the redshift range z=0.3-0.5 at dec<-40. This category of clusters has already received tremendous attention as witnessed by a series of studies on cluster structure, lensing properties, SZ observations, galaxy population and dynamics. They are also the most important cosmological probes at the intermediate redshift to trace large-scale structure evolution, and to constrain cosmological parameters. Therefore we propose the XMM observations of these 10 luminous known clusters to a sufficient depth to precisely assess their physical properties.

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