Exploring Supermassive Black Hole Accretion in z>3 AGN, Obscured AGN and XBONGs

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Cosmology, Extragalactic Deep Fields And Area Surveys, Bootes1, Bootes2, Bootes3, Bootes4, Bootes5, Bootes1, Bootes1, Bootes8, Bootes9, Xmm-Newton Proposal Id #05527009

Scientific paper

We propose to measure accurate X-ray fluxes and spectra for large samples of high redshift luminous AGN, XBONGS, and large numbers of obscured Type 2 sources, found from our Chandra XBootes survey. We obtained optical spectra for 258 XBONGs and 150 z>3 AGN and identified 640 X-ray luminous Type 2 AGN. We selected XMM-Newton fields with a high AGN density and will accurately determine X-ray luminosities and average spectra for 70 z>3 AGN, thus tripling the number of well studied high z X-ray AGN. For the sample of 220 Type 2 AGN, we will examine the distribution of n_H values and estimate the fraction of very highly obscured AGN. For XBONGS, we will determine if they represent a radiatively inefficient accretion mode with an intermediate Eddington ratio.

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