THE CHANDRA COSMOS LEGACY SURVEY: CLUSTERING OF X-RAY-SELECTED AGNs AT 2.9 ≤ z ≤ 5.5 USING PHOTOMETRIC REDSHIFT PROBABILITY DISTRIBUTION FUNCTIONS

被引:22
作者
Allevato, V. [1 ,2 ]
Civano, F. [3 ,4 ]
Finoguenov, A. [1 ,2 ]
Marchesi, S. [3 ,4 ,5 ]
Shankar, F. [6 ]
Zamorani, G. [7 ]
Hasinger, G. [8 ]
Salvato, M. [9 ]
Miyaji, T. [10 ]
Gilli, R. [5 ]
Cappelluti, N. [3 ]
Brusa, M. [5 ,7 ]
Suh, H. [8 ]
Lanzuisi, G. [5 ,7 ]
Trakhtenbrot, B. [11 ]
Griffiths, R. [12 ]
Vignali, C. [5 ,7 ]
Schawinski, K. [11 ]
Karim, A. [13 ]
机构
[1] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, Helsinki 00014, Finland
[2] Univ Maryland, 1000 Hilltop Circle, Baltimore, MD 21250 USA
[3] Yale Ctr Astron & Astrophys, 260 Whitney Ave, New Haven, CT 06520 USA
[4] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[5] Univ Bologna, Dipartimento Fis & Astron, Alma Mater Studiorum, Viale Berti Pichat 6-2, I-40127 Bologna, Italy
[6] Univ Southampton, Dept Phys & Astron, Highfield SO17 1BJ, England
[7] NAF Osservatorio Astron Bologna, Via Ranzani 1, I-40127 Bologna, Italy
[8] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
[9] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany
[10] Univ Nacl Autonoma Mexico, Inst Astron, Ensenada, Baja California, Mexico
[11] ETH, Inst Astron, Dept Phys, Wolfgang Pauli Str 27, CH-8093 Zurich, Switzerland
[12] Univ Hawaii, 200 W Kawili St, Hilo, HI 96720 USA
[13] Univ Bonn, Argelander Inst Astron, Hugel 71, D-53121 Bonn, Germany
基金
瑞士国家科学基金会;
关键词
dark matter; galaxies: active; large-scale structure of universe; surveys; X-rays: general; SUPERMASSIVE BLACK-HOLES; ACTIVE GALACTIC NUCLEI; WIDE-FIELD SURVEY; CROSS-CORRELATION FUNCTION; DARK-MATTER HALOES; HOST GALAXIES; STAR-FORMATION; QUASARS; EVOLUTION; MODEL;
D O I
10.3847/0004-637X/832/1/70
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the measurement of the projected and redshift-space two-point correlation function (2pcf) of the new catalog of Chandra COSMOS-Legacy active galactic nucleus (AGN) at 2.9 <= z <= 5.5 (<L-bol> similar to 10(46) erg s(-1)) using the generalized clustering estimator based on phot-z probability distribution functions in addition to any available spec-z. We model the projected 2pcf, estimated using pi(max) = 200 h(-1) Mpc with the two-halo term and we derive a bias at z similar to 3.4 equal to b. =. 6.6(+0.60) -(0.55), which corresponds to a typical mass of the hosting halos of log M-h. =. 12.83(+0.12) -(0.11) h(-1)M circle dot. A similar bias is derived using the redshift-space 2pcf, modeled including the typical phot-z error sigma(z). =. 0.052 of our sample at z >= 2.9. Once we integrate the projected 2pcf up to pi(max). =. 200 h(-1) Mpc, the bias of XMM and Chandra COSMOS at z =. 2.8 used in Allevato et al. is consistent with our results at higher redshifts. The results suggest only a slight increase of the bias factor of COSMOS AGNs at z greater than or similar to 3 with the typical hosting halo mass of moderate-luminosity AGNs almost constant with redshift and equal to log M-h = 12.92(+0.-13) (0.18) at z - 2.8 and log M-h - 12.83(+0.11) (-0.12) at z similar to 3.4, respectively. The observed redshift evolution of the bias of COSMOS AGNs implies that moderate-luminosity AGNs. still inhabit group-sized halos at z greater than or similar to 3, but slightly less massive than observed in different independent studies using X-ray AGNs. at z less than or similar to 2.
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页数:10
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