Evidence for a large fraction of Compton-thick quasars at high redshift

Details Evidence for a large fraction of Compton-thick quasars at high redshift Evidence for a large fraction of Compton-thick quasars at high redshift

2006-11-23

arxiv.org/abs/astro-ph/0611739v2

Mon.Not.Roy.Astron.Soc.Lett.379:L6-L10,2007

Astronomy and Astrophysics

Astrophysics

6 pages, 2 colour figures. Accepted by MNRAS. Full resolution version and supplementary figures can be found at: http://www.

Scientific paper

10.1111/j.1745-3933.2007.00323.x

Using mid-infrared and radio selection criteria, we pre-select a sample of candidate high-redshift type-2 quasars in the Subaru XMM-Newton Deep Field (SXDF). To filter out starburst contaminants, we use a bayesian method to fit the spectral energy distributions (SEDs) between 24-microns and B-band, obtain photometric redshifts, and identify the best candidates for high-z type-2 quasars. This leaves us with 12 z_phot >= 1.7 type-2 quasar candidates in an area ~0.8 deg^2, of which only two have secure X-ray detections. The two detected sources have estimated column densities N_H~2 & 3x10^27 m^-2, i.e. heavily obscured but Compton-thin quasars. Given the large bolometric luminosities and redshifts of the undetected objects, the lack of X-ray detections suggests extreme absorbing columns N_H >= 10^28 m^-2 are typical. We have found evidence for a population of ``Compton-thick'' high-redshift type-2 quasars, at least comparable to, and probably larger than the type-1 quasar population, although spectroscopic confirmation of their AGN nature is important.

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