Computer Science
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop...14m&link_type=abstract
XMM-Newton Proposal ID #06703511
Computer Science
Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rxcj1423.1+2615, Rxcj1454.4+1622, Rxcj1615.5+1927, Rxcj1617.5+3458, Rxcj1627.3+4240, Rxcj1654.3+2334, Rxcj1658.0+2751, Rxcj1722.2+3042, Rxcj1109.7+2145, Rxcj1121.7+0249, Rxcj1132.3+5558
Scientific paper
We propose an XMM-Newton survey of a complete X-ray selected sample of nearby galaxy groups. The groups have been selected to overlap with the Sloan Digital Sky Survey. The XMM observations will provide a vital comparison sample to X-ray selected group samples being studied at high redshift. We will use the XMM observations to: 1) Determine the properties of the intragroup medium in a representative sample of X-ray groups; 2) Study the evolution of the galaxy population in X-ray groups from z=1 to the present; 3) Determine the formation timescales of brightest group galaxies and 4) Compare the AGN populations in X-ray groups to clusters.
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