XMM-Newton Proposal 03025819

Details XMM-Newton Proposal 03025819 XMM-Newton Proposal 03025819

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...96a&link_type=abstract

XMM-Newton Proposal ID #03025819

Physics

Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Rxj2328.8+1453, Rxj1002.6-0808, Rxj0957.8+6534, Rxj2359.5-3211, Rxj1311.5-0551, Rxj2146.0+0423, Rxj0522.2-3625, Rxj0030.5+2618, Rxj0221.1+1958, Ms1241.5+1710, Rxj1003.0+3254, Rxj0856.1+3756, Rxj1206.2-0848, Xmm-Newton Proposal 03025819

Scientific paper

We propose to observe a large unbiased sample of distant (z~0.5) clusters. The clusters in the sample cover the wide dynamic range in mass (kT = [2.5-12] keV) necessary to fully assess the evolution of cluster scaling and structural properties. This will provide unique insight into the physics of structure formation, both for the dark matter and the baryonic components (e.g. how non-gravitational processes drive departures from the predictions of the simplest self-similar model of gravitational collapse). We propose that the observations be conducted as a Public Large project.

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