We present results from a spectral analysis of a sample of high-redshift (z > 3) X-ray-selected active galactic nucleus (AGN) in the 4-Ms Chandra Deep Field-South (CDF-S), the deepest X-ray survey to date. The sample is selected using the most recent spectroscopic and photometric information available in this field. It consists of 34 sources with median redshift z = 3.7, 80 median net counts in the 0.5-7 keV band and median rest-frame absorption-corrected luminosity L2-10 keV ≈ 1.5 × 1044 erg s-1. Spectral analysis for the full sample is presented and the intrinsic column density distribution, corrected for observational biases using spectral simulations, is compared with the expectations of X-ray background (XRB) synthesis models. We find that ≈57 per cent of the sources are highly obscured (NH > 1023 cm-2). Source number counts in the 0.5-2 keV band down to flux F0.5-2 keV ≈ 4 × 10-17 erg s-1 cm-2 are also presented. Our results are consistent with a decline of the AGN space density at z > 3 and suggest that, at those redshifts, the AGN obscured fraction is in agreement with the expectations of XRB synthesis models.
The high-redshift (z>3) active galactic nucleus population in the 4-Ms Chandra Deep Field-South / Vito F.; Vignali C.; Gilli R.; Comastri A.; Iwasawa K.; Brandt W.N.; Alexander D.M.; Brusa M.; Lehmer B.; Bauer F.E.; Schneider D.P.; Xue Y.Q.; Luo B.. - In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. - ISSN 0035-8711. - STAMPA. - 428:(2013), pp. 354-369. [10.1093/mnras/sts034]
The high-redshift (z>3) active galactic nucleus population in the 4-Ms Chandra Deep Field-South
VITO, FABIO;VIGNALI, CRISTIAN;BRUSA, MARCELLA;
2013
Abstract
We present results from a spectral analysis of a sample of high-redshift (z > 3) X-ray-selected active galactic nucleus (AGN) in the 4-Ms Chandra Deep Field-South (CDF-S), the deepest X-ray survey to date. The sample is selected using the most recent spectroscopic and photometric information available in this field. It consists of 34 sources with median redshift z = 3.7, 80 median net counts in the 0.5-7 keV band and median rest-frame absorption-corrected luminosity L2-10 keV ≈ 1.5 × 1044 erg s-1. Spectral analysis for the full sample is presented and the intrinsic column density distribution, corrected for observational biases using spectral simulations, is compared with the expectations of X-ray background (XRB) synthesis models. We find that ≈57 per cent of the sources are highly obscured (NH > 1023 cm-2). Source number counts in the 0.5-2 keV band down to flux F0.5-2 keV ≈ 4 × 10-17 erg s-1 cm-2 are also presented. Our results are consistent with a decline of the AGN space density at z > 3 and suggest that, at those redshifts, the AGN obscured fraction is in agreement with the expectations of XRB synthesis models.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
