Computer Science
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..107s&link_type=abstract
XMM-Newton Proposal ID #04027811
Computer Science
Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, J101806.68+0005, J125027.42+0013, J003937.83-0019, J023140.97-0110, J155855.79+0248, J233604.04+0004, J081040.29+4812, J090624.6+00575, J142041.03+0159, J150754.38+0108, J170007.17+3750, Xmm-Newton Proposal 04027811
Scientific paper
From the SDSS radio-loud AGN sample of Best et al. (2005) we extracted a volume-limited (z<0.1) sample of 11 Broad Line Radio Galaxies, with X-ray luminosities in the range 10^41-10^43 erg/s, 3 orders of magnitude lower than classical BLRGs, and matching most Seyferts. The XMM observations of this new sample will allow us to: 1) measure the X-ray continua; 2) test multiwavelength correlations valid for bright BLRGs; and 3) constrain the optical-to-X-ray SEDs. We will constrain the nature of the accretion flow and relative importance of the jet in these sources,and compare to luminous radio-loud and radio-quiet AGNs to uncover the fundamental parameters that determine the properties of radio-loud AGN.
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