XMM-Newton Proposal 03013405

Details XMM-Newton Proposal 03013405 XMM-Newton Proposal 03013405

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...46b&link_type=abstract

XMM-Newton Proposal ID #03013405

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Sdss 0839+5112, Class J0918+063, Pmn J0214-0518, Pmn J2219-2719, First 1309+5733, Xmm-Newton Proposal 03013405

Scientific paper

We propose to extend our systematic X-ray studies of the most distant known quasars with XMM-Newton spectroscopic observations of six radio-loud quasars (RLQs) at z = 3.63-4.39. Our targets are more representative of the overall RLQ population than the small number of highly radio-loud blazars studied at high redshift, and we have detected all targets in exploratory Chandra observations. We will study X-ray absorption in the quasars' environments to determine if it is common among typical RLQs at high redshift. We will also measure X-ray continuum shapes and search for variability, clustered AGN, and X-ray jets.

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