XMM-Newton Proposal 02032703

Details XMM-Newton Proposal 02032703 XMM-Newton Proposal 02032703

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..173p&link_type=abstract

XMM-Newton Proposal ID #02032703

Computer Science

Rxj094144+385434, Rxj121803+470854, Rxj124913-055906, Xmm-Newton Proposal 02032703

Scientific paper

According to galaxy formation models, cluster ellipticals formed in high density regions through hierarchical merging of gas rich sub-components. In local ellipticals, the strong correlation observed between black hole and bulge mass implies that galaxy formation is inextricably linked to the build up of supermassive black holes. We have found 4 high redshift, X-ray luminous, but heavily absorbed AGN, embedded in strong bursts of star formation revealed in the submillimetre. Our SCUBA survey shows that the immediate vicinities of these objects contain large overdensities of ultraluminous star-forming galaxies which will evolve to form clusters. Here we propose to use XMM to observe the early evolutionary phases of QSOs in these proto-clusters.

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