XMM-Newton Proposal 02034508

Details XMM-Newton Proposal 02034508 XMM-Newton Proposal 02034508

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..181a&link_type=abstract

XMM-Newton Proposal ID #02034508

Physics

Rx J0858.4+1357, Rx J2202.7-1902, Vmf116, Rx J2359.5-3211, Vmf117, Vmf162/Vmf161, Vmf204, Vmf98, Xmm-Newton Proposal 02034508

Scientific paper

We propose to observe a large unbiased sample of distant (z[0.4-0.6]) galaxy 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). The project is defined so to make maximum use of XMM and Chandra existing observations. We propose that the observations are conducted as a Public Large project.

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