XMM-Newton Proposal 03058007

Details XMM-Newton Proposal 03058007 XMM-Newton Proposal 03058007

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..187p&link_type=abstract

XMM-Newton Proposal ID #03058007

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Mz 3849, Mz 3541, Mz 10451, Mz 4940, Mz 9307, Mz 4592, Mz 5293, Xmm-Newton Proposal 03058007

Scientific paper

Despite the importance of galaxy groups as the most common galaxy environment, and the likely repository of the majority of baryons in the Universe, no study of the dynamics and baryon contents of an unbiased sample has ever been conducted. We have begun a project to remedy this, targetting a sample of 25 groups derived from the 2dF galaxy redshift survey with XMM, in combination with the large IMACS imaging spectrograph. The resulting dataset will provide a unique resource for studying the structure and evolution of groups, and the way in which group galaxies interact with their evolving environment. Optical imaging and IMACS spectroscopy of these is progressing well, and we request 20 ksec observations of seven groups, to add to the three awarded in AO-3.

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