XMM-Newton Proposal 02021403

Details XMM-Newton Proposal 02021403 XMM-Newton Proposal 02021403

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop..114p&link_type=abstract

XMM-Newton Proposal ID #02021403

Physics

Br B1202-0725, Lbqs B0018-0220, Pss J2322+1944, Xmm-Newton Proposal 02021403

Scientific paper

Observations of luminous, high-redshift quasars in the submillimetre band suggest that a high fraction of these AGN coexist alongside powerful, dust-enshrouded star formation in their host galaxies. They thus bear all the hallmarks of youthful galaxies, inhabiting an environment rich in gas and dust. We propose to obtain sensitive XMM--Newton spectroscopy of high-redshift, submm-luminous quasars from our intensive, multiwavelength study. This will establish whether there is any correlation between anomalous X-ray spectra (e.g. intrinsic absorption) and the presence of starbursts and/or large masses of molecular gas. This has significant implications for our understanding of the relation between the formation of AGN and their massive host galaxies.

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