Black hole growth and starburst activity at z=0.6-4 in the Chandra Deep Field South Host galaxies properties of obscured AGN

被引：94

作者：

Brusa, M. ^{[1
]}

Fiore, F. ^{[2
]}

Santini, P. ^{[2
]}

Grazian, A. ^{[2
]}

Comastri, A. ^{[3
]}

Zamorani, G. ^{[3
]}

Hasinger, G. ^{[1
,4
]}

Merloni, A. ^{[5
]}

Civano, F. ^{[6
]}

Fontana, A. ^{[2
]}

Mainieri, V. ^{[7
]}

机构：

[1] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

[2] Osserv Astron Roma, INAF, I-00040 Rome, Italy

[3] Osservatorio Astron Bologna, INAF, I-40127 Bologna, Italy

[4] Max Planck Inst Plasma Phys, D-85748 Garching, Germany

[5] Excellence Cluster Universe, D-85748 Garching, Germany

[6] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[7] European So Observ, D-85748 Garching, Germany

来源：

ASTRONOMY & ASTROPHYSICS | 2009年 / 507卷 / 03期

关键词：

galaxies: active; galaxies: starburst; X-rays: galaxies; RAY SPECTRAL PROPERTIES; POINT-SOURCE CATALOGS; GOODS-MUSIC SAMPLE; X-RAY; GALACTIC NUCLEI; MASSIVE GALAXIES; STAR-FORMATION; HIGH-REDSHIFT; LUMINOSITY FUNCTION; COSMOS FIELD;

D O I：

10.1051/0004-6361/200912261

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Aims. The co-evolution of host galaxies and the active black holes which reside in their centre is one of the most important topics in modern observational cosmology. Here we present a study of the properties of obscured active galactic nuclei (AGN) detected in the CDFS 1 Ms observation and their host galaxies. Methods. We limited the analysis to the MUSIC area, for which deep K-band observations obtained with ISAAC@VLT are available, ensuring accurate identifications of the counterparts of the X-ray sources as well as reliable determination of photometric redshifts and galaxy parameters, such as stellar masses and star formation rates. In particular, we: 1) refined the X-ray/infrared/optical association of 179 sources in the MUSIC area detected in the Chandra observation; 2) studied the host galaxies observed and rest frame colors and properties. Results. We found that X-ray selected (L-X greater than or similar to 10(42) erg s(-1)) AGN show Spitzer colors consistent with both AGN and starburst dominated infrared continuum; the latter would not have been selected as AGN from infrared diagnostics. The host galaxies of X-ray selected obscured AGN are all massive (M-* > 10(10) M-circle dot) and, in 50% of the cases, are also actively forming stars (1/SSFR < t(Hubble)) in dusty environments. The median L/L-Edd value of the active nucleus is between 2% and 10% depending on the assumed M-BH/M-* ratio. Finally, we found that the X-ray selected AGN fraction increases with the stellar mass up to a value of similar to 30% at z > 1 and M-* > 3 x 10(11) M-circle dot, a fraction significantly higher than in the local Universe for AGN of similar luminosities.

引用

页码：1277 / U119

页数：20

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