Galaxy evolution in the large scale structure around two PISCES galaxy clusters

Details Galaxy evolution in the large scale structure around two PISCES galaxy clusters Galaxy evolution in the large scale structure around two PISCES galaxy clusters

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..110m&link_type=abstract

XMM-Newton Proposal ID #05028601

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Cl0016+1609 Off, Xmm-Newton Proposal 05028601

Scientific paper

The effect of environment is an essential, but poorly understood ingredient in galaxy formation. We propose to measure the gas and dark matter in the clumps and filaments around two massive distant galaxy clusters. By combining high quality XMM data with our existing wide-field optical-NIR imaging and spectroscopy we will perform a census of the baryons in the large scale structure around these clusters and measure the effects of environment on the fundamental physical properties of the member galaxies.

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