Computer Science
Scientific paper
Oct 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008xmm..prop...42b&link_type=abstract
XMM-Newton Proposal ID #06017419
Computer Science
Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Igr J00333+6122, Ngc788, Igr J07565-4139, Swift J0917.2+5, Igr J09523-6231, Igr J12026-5349, Igr J13109-5552, Igr J14515-5542, Igr J16024-6107, Igr J16119-6036, Igr J16185-5928, Igr J16385-2057, Swift J1656.3-3, Grs 1734-292, 2E1853.7+1534, Ngc6814, S52116+5058, Swift J2127.4+5
Scientific paper
We propose to observe with XMM-Newton all 19 AGN (from a complete sample of 74 INTEGRAL selected objects), for which no or limited spectral information are available below 10 keV. XMM observations will allow us to cover the missing information in the X-ray band and to characterize the broad band emission of these newly discovered sources. We emphasize here the hard X-ray selection of our sources and the unique role of INTEGRAL data in providing spectral information above 10 keV. This is the continuation of 3 previous successful XMM proposals, which have so far provided X-ray data for a number of INTEGRAL AGNs. We estimate a single source exposure in the range of 15-30 ks, for a total time of 345 ks, therefore we submit an XMM Large Program.
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