We present the high-redshift (3 <z < 5.3) 0.5-2 keV number counts and the 2-10 keV (rest-frame) space density of X-ray-selected active galactic nuclei (AGNs) detected in the Chandra Cosmic Evolution Survey. The sample comprises 81 X-ray-detected sources with available spectroscopic (31) and photometric (50) redshifts plus 20 sources with a formal z phot < 3 but with a broad photometric redshift probability distribution, such that z phot + 1σ > 3. Eighty-one sources are selected in the 0.5-2 keV band, fourteen are selected in the 2-10 keV and six in the 0.5-10 keV bands. We sample the high-luminosity (log L (2-10 keV) > 44.15 erg s-1) space density up to z ~ 5 and a fainter luminosity range (43.5 erg s-1 < log L (2-10 keV) < 44.15 erg s-1) than previous studies, up to z = 3.5. We weighted the contribution to the number counts and the space density of the sources with photometric redshift by using their probability of being at z > 3. We find that the space density of high-luminosity AGNs declines exponentially at all the redshifts, confirming the trend observed for optically selected quasars. At lower luminosity, the measured space density is not conclusive, and a larger sample of faint sources is needed. Comparisons with optical luminosity functions and black hole formation models are presented together with prospects for future surveys.
The population of high-redshift Active Galactic Nuclei in the Chandra-COSMOS survey / Civano F.; Brusa M.; Comastri A.; Elvis M.; Salvato M.; Zamorani G.; Capak P.; Fiore F.; Gilli R.; Hao H.; Ikeda H.; Kakazu Y.; Kartaltepe J.S.; Masters D.; Miyaji T.; Mignoli M.; Puccetti S.; Shankar F.; Silverman J.; Vignali C.; Zezas A.; Koekemoer A.M.. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - STAMPA. - 741:(2011), pp. 91-101. [10.1088/0004-637X/741/2/91]
The population of high-redshift Active Galactic Nuclei in the Chandra-COSMOS survey
BRUSA, MARCELLA;VIGNALI, CRISTIAN;
2011
Abstract
We present the high-redshift (3I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.