A Complete Sample of the Brightest Type 2 AGN in the SDSS

Details A Complete Sample of the Brightest Type 2 AGN in the SDSS A Complete Sample of the Brightest Type 2 AGN in the SDSS

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..155h&link_type=abstract

XMM-Newton Proposal ID #05041018

Physics

Active Galactic Nuclei, Quasars, Bl-Lac Objects, X-Ray Background, Sdss0824+2959, Sdss0959+1259, Sdss0053-0846, Sdss1437+3634, Sdss1238+0927, Sdss0804+2345, Sdss1157+5249, Sdss1136+5657, Sdss0800+2636, Sdss1123+4703, Sdss1147+5226, Sdss1346+6423, Sdss1323+4318, Sdss1018+3722, Sdss1111+0228, Xmm-Newton Proposal 05041018

Scientific paper

We propose to obtain XMM-Newton data for a complete sample of the 20 brightest Type 2 AGN drawn from ~100000 low-z AGN in the SDSS DR4. The sample members have a flux in the [OIII]5007 emission line of at least 4E-14 ergs/cm2/s. This sample has approved Spitzer spectroscopic observations and each galaxy has a wealth of information about the AGN and its host galaxy derived homogeneously from the SDSS (including the black hole mass, [OIII] luminosity, and Eddington ratio for the AGN and the mass, structure, and stellar content of the galaxy). We will use these combined data to determine the fraction of Compton-thick AGN and to determine whether they differ systematically in terms of the properties of the AGN and the host galaxy, providing new insights into AGN physics.

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