Computer Science
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop..195g&link_type=abstract
XMM-Newton Proposal ID #06746602
Computer Science
Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Slj1201.7-0331
Scientific paper
We propose XMM observations (totaling 107 ks) of 6 galaxy clusters in the redshift range 0.3 < z < 0.6 selected in a Subaru weak lensing (WL) survey. This will complete a sample of 8 clusters that will be used to study systematically the X-ray properties of clusters detected independently of their baryonic content. We will investigate biases in cluster selection techniques for high-z clusters, compare the high-z scaling relations of the X-ray properties (e.g. Lx, kT, Mgas, Yx) of WL selected clusters to those of X-ray selected clusters, investigate the evolution of the properties of WL selected clusters from the local to high redshift universe and study their morphology/structure.
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