XMM-Newton Proposal 03024003

Details XMM-Newton Proposal 03024003 XMM-Newton Proposal 03024003

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...86s&link_type=abstract

XMM-Newton Proposal ID #03024003

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, 0723+679, Xmm-Newton Proposal 03024003

Scientific paper

We propose to perform EPIC spectroscopy and OM photometry of 4 powerful radio-loud quasars with known large scale radio/X properties, and where an Fe line was detected at 6--7 keV in our short Chandra observations. The proposed observations will enable us to: 1) Quantify the Fe line profile and determine its origin; 2) Determine the shape of the underlying X-ray continuum; and 3) Constrain the broad-band SEDs, in particular search for thermal UV emission which is asignature of standard disks. Ultimately, this will allow us to discern the relative roles of beamed and isotropic radiation from the cores of RL AGN, yielding information on the jet-disk connection and on the origin of the RL/RQ AGN division.

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