Testing Radio-loud vs. Radio-quiet AGN Unification

Details Testing Radio-loud vs. Radio-quiet AGN Unification Testing Radio-loud vs. Radio-quiet AGN Unification

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010xmm..prop...32t&link_type=abstract

XMM-Newton Proposal ID #06708806

Computer Science

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Pks 2251+11, 3C 215, 3C 411

Scientific paper

We propose EPIC pn observations of four Broad-Line Radio Galaxies previously studied by us with ASCA. The immediate goals of the observations are to 1) confirm (3C 303) and search for (PKS 2251+11, 3C 215, 3C 411) the Fe Kalpha emission line and study its profile; and 2) constrain absorption at soft energies. On the longer term, these observations will expand the current number of radio-loud AGNs with high quality X-ray spectra and allow a systematic comparison to Seyferts, testing in a meaningful way specific models for the radio-quiet/radio-loud AGN distribution.

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