X-RAY SELECTED AGN HOST GALAXIES ARE SIMILAR TO INACTIVE GALAXIES OUT TO z=3: RESULTS FROM CANDELS/CDF-S

被引：49

作者：

Rosario, D. J. ^{[1
]}

Mozena, M. ^{[2
,3
]}

Wuyts, S. ^{[1
]}

Nandra, K. ^{[1
]}

Koekemoer, A. ^{[4
]}

McGrath, E. ^{[5
]}

Hathi, N. P. ^{[6
]}

Dekel, A. ^{[7
]}

Donley, J. ^{[8
]}

Dunlop, J. S. ^{[9
]}

Faber, S. M. ^{[2
,3
]}

Ferguson, H. ^{[4
]}

Giavalisco, M. ^{[10
]}

Grogin, N. ^{[4
]}

Guo, Y. ^{[10
]}

Kocevski, D. D. ^{[11
]}

Koo, D. C. ^{[2
,3
]}

Laird, E. ^{[12
]}

Newman, J. ^{[13
]}

Rangel, C. ^{[12
]}

Somerville, R. ^{[14
]}

机构：

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

[2] Univ Calif Santa Cruz, Dept Astron, Santa Cruz, CA 95064 USA

[3] Univ Calif Santa Cruz, UCO Lick Observ, Santa Cruz, CA 95064 USA

[4] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[5] Colby Coll, Dept Phys, Waterville, ME 04901 USA

[6] Observ Carnegie Inst Washington, Pasadena, CA 91101 USA

[7] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel

[8] Los Alamos Natl Lab, Los Alamos, NM 87545 USA

[9] Royal Observ, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland

[10] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA

[11] Univ Kentucky, Dept Phys & Astron, Lexington, KY 40506 USA

[12] Univ London Imperial Coll Sci Technol & Med, Dept Phys, London SW7 2AZ, England

[13] Univ Pittsburgh, Dept Phys & Astron, Pittsburgh, PA 15260 USA

[14] Rutgers State Univ, Dept Phys & Astron, Piscataway, NJ 08854 USA

来源：

ASTROPHYSICAL JOURNAL | 2013年 / 763卷 / 01期

基金：

美国国家科学基金会;

关键词：

galaxies: active; galaxies: photometry; infrared: galaxies; surveys; X-rays: galaxies; ACTIVE GALACTIC NUCLEI; SUPERMASSIVE BLACK-HOLES; DEEP FIELD-SOUTH; STELLAR POPULATION SYNTHESIS; SIMILAR-TO; STAR-FORMATION; COLOR-MAGNITUDE; COSMOLOGICAL FRAMEWORK; OPTICAL SPECTROSCOPY; PHOTOMETRIC REDSHIFT;

D O I：

10.1088/0004-637X/763/1/59

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We use multi-band spatially resolved photometry from the Cosmic Assembly Near-IR Deep Legacy Survey in the 4 Ms Chandra Deep Field-South to explore the nuclear and extended colors, color gradients, and stellar populations of the host galaxies of X-ray selected active galactic nuclei (AGNs) out to z = 3. Based on a study of their central light, we develop X-ray based criteria to exclude objects with strong AGN contamination. We use stellar masses from the FIREWORKS database to understand and account for stellar mass selection effects and carefully study, for the first time, the resolved host galaxy properties of AGNs at z similar to 2 in their rest-frame optical light without substantial nuclear contamination. AGN hosts span a sizable range of stellar masses, colors, and color gradients at these redshifts. Their colors, color gradients, and stellar population properties are very similar to inactive galaxies of the same stellar mass. At z similar to 1, we find a slightly narrower range in host colors compared to inactive galaxies, as well as hints of more recent star formation. These differences are weaker or non-existent among AGN hosts at z similar to 2. We discuss the importance of AGN-driven feedback in the quenching of galaxies at z greater than or similar to 1 and speculate on possible evolution in the relationship between black hole accretion and the host galaxy toward high redshifts.

引用

页数：19

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