We present results from a spectral analysis of a sample of 34 high-redshift (z > 3) X-ray selected AGN in the 4 Ms Chandra Deep Field South, the deepest X-ray survey to date. The intrinsic column density distribution, corrected for observational bi- ases using spectral simulations, and the source number counts down to flux F0.5−2keV∼ 4 × 10−17 erg s−1 cm−2 are compared with the expectations from X-ray background synthesis models. All the results are presented and discussed in Vito et al. (2013).
Vito F., Vignali C., Gilli R., Comastri A., Iwasawa K., Brandt W.N., et al. (2013). The z > 3 AGN population in the 4 Ms CDFS. Pisa : Mem. S.A.It.
The z > 3 AGN population in the 4 Ms CDFS
VITO, FABIO;VIGNALI, CRISTIAN;BRUSA, MARCELLA;
2013
Abstract
We present results from a spectral analysis of a sample of 34 high-redshift (z > 3) X-ray selected AGN in the 4 Ms Chandra Deep Field South, the deepest X-ray survey to date. The intrinsic column density distribution, corrected for observational bi- ases using spectral simulations, and the source number counts down to flux F0.5−2keV∼ 4 × 10−17 erg s−1 cm−2 are compared with the expectations from X-ray background synthesis models. All the results are presented and discussed in Vito et al. (2013).I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
