The Chandra COSMOS Legacy Survey: Energy Spectrum of the Cosmic X-Ray Background and Constraints on Undetected Populations

被引:74
作者
Cappelluti, Nico [1 ,2 ,3 ]
Li, Yanxia [1 ,2 ,3 ,4 ]
Ricarte, Angelo [3 ]
Agarwal, Bhaskar [1 ,2 ,3 ]
Allevato, Viola [5 ]
Ananna, Tonima Tasnim [1 ,2 ,3 ]
Ajello, Marco [6 ]
Civano, Francesca [7 ]
Comastri, Andrea [8 ]
Elvis, Martin [7 ]
Finoguenov, Alexis [5 ,9 ]
Gilli, Roberto [8 ]
Hasinger, Guenther [4 ]
Marchesi, Stefano [6 ]
Natarajan, Priyamvada [1 ,2 ,3 ]
Pacucci, Fabio [2 ]
Treister, E. [10 ]
Urry, C. Megan [1 ,2 ,3 ]
机构
[1] Yale Ctr Astron & Astrophys, POB 208121, New Haven, CT 06504 USA
[2] Yale Univ, Dept Phys, POB 208121, New Haven, CT 06520 USA
[3] Yale Univ, Dept Astron, POB 208101, New Haven, CT 06520 USA
[4] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
[5] Univ Helsinki, Dept Phys, Gustaf Hallstromin Katu 2a, FI-00014 Helsinki, Finland
[6] Clemson Univ, Dept Phys & Astron, Kinard Lab Phys, Clemson, SC 29634 USA
[7] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[8] Osservatorio Astron Bologna, INAF, Via Ranzani 1, I-40127 Bologna, Italy
[9] Max Planck Inst Extraterr Phys, Postfach 1312, D-85741 Garching, Germany
[10] Pontificia Univ Catolica Chile, Fac Fis, Inst Astrofis, Casilla 306, Santiago 22, Chile
基金
美国国家科学基金会;
关键词
catalogs; infrared: diffuse background; quasars: supermassive black holes; surveys; X-rays: diffuse background; ACTIVE GALACTIC NUCLEI; POINT-SOURCE CATALOG; 1ST BLACK-HOLES; XMM-NEWTON; EVOLUTION; ABSORPTION; MODEL; IDENTIFICATION; FLUCTUATIONS; LUMINOSITY;
D O I
10.3847/1538-4357/aa5ea4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using Chandra observations in the 2.15 deg(2) COSMOS-legacy field, we present one of the most accurate measurements of the Cosmic X-ray Background (CXB) spectrum to date in the [0.3-7] keV energy band. The CXB has three distinct components: contributions from two Galactic collisional thermal plasmas at kT similar to 0.27 and 0.07 keV and an extragalactic power law with a photon spectral index Gamma = 1.45 +/- 0.02. The 1 keV normalization of the extragalactic component is 10.91 +/- 0.16 keV cm(-2) s(-1) sr(-1) keV(-1). Removing all X-ray-detected sources, the remaining unresolved CXB is best fit by a power law with normalization 4.18 +/- 0.26 keV cm(-2) s(-1) sr(-1) keV(-1) and photon spectral index Gamma = 1.57 +/- 0.10. Removing faint galaxies down to i(AB) similar to 27-28 leaves a hard spectrum with Gamma similar to 1.25 and a 1 keV normalization of similar to 1.37 keV cm(-2) s(-1) sr(-1) keV(-1). This means that similar to 91% of the observed CXB is resolved into detected X-ray sources and undetected galaxies. Unresolved sources that contribute similar to 8%-9% of the total CXB show marginal evidence of being harder and possibly more obscured than resolved sources. Another similar to 1% of the CXB can be attributed to still undetected star-forming galaxies and absorbed active galactic nuclei. According to these limits, we investigate a scenario where early black holes totally account for non-source CXB fraction and constrain some of their properties. In order to not exceed the remaining CXB and the z similar to 6 accreted mass density, such a population of black holes must grow in Compton-thick envelopes with N-H > 1.6 x 10(25) cm(-2) and form in extremely low-metallicity environments (Z(circle dot)) similar to 10(-3).
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页数:8
相关论文
共 61 条
[1]   COSMIC X-RAY BACKGROUND AND EARTH ALBEDO SPECTRA WITH SWIFT BAT [J].
Ajello, M. ;
Greiner, J. ;
Sato, G. ;
Willis, D. R. ;
Kanbach, G. ;
Strong, A. W. ;
Diehl, R. ;
Hasinger, G. ;
Gehrels, N. ;
Markwardt, C. B. ;
Tueller, J. .
ASTROPHYSICAL JOURNAL, 2008, 689 (02) :666-677
[2]  
Arnaud KA, 1996, ASTR SOC P, V101, P17
[3]   LIFTING THE VEIL ON OBSCURED ACCRETION: ACTIVE GALACTIC NUCLEI NUMBER COUNTS AND SURVEY STRATEGIES FOR IMAGING HARD X-RAY MISSIONS [J].
Ballantyne, D. R. ;
Draper, A. R. ;
Madsen, K. K. ;
Rigby, J. R. ;
Treister, E. .
ASTROPHYSICAL JOURNAL, 2011, 736 (01)
[4]   The cosmic evolution of hard X-ray-selected active galactic nuclei [J].
Barger, AJ ;
Cowie, LL ;
Mushotzky, RF ;
Yang, Y ;
Wang, WH ;
Steffen, AT ;
Capak, P .
ASTRONOMICAL JOURNAL, 2005, 129 (02) :578-609
[5]   Chandra ACIS-I particle background: an analytical model [J].
Bartalucci, I. ;
Mazzotta, P. ;
Bourdin, H. ;
Vikhlinin, A. .
ASTRONOMY & ASTROPHYSICS, 2014, 566
[6]   THE X-RAY STAR FORMATION STORY AS TOLD BY LYMAN BREAK GALAXIES IN THE 4 Ms CDF-S [J].
Basu-Zych, Antara R. ;
Lehmer, Bret D. ;
Hornschemeier, Ann E. ;
Bouwens, Rychard J. ;
Fragos, Tassos ;
Oesch, Pascal A. ;
Belczynski, Krzysztof ;
Brandt, W. N. ;
Kalogera, Vassiliki ;
Luo, Bin ;
Miller, Neal ;
Mullaney, James R. ;
Tzanavaris, Panayiotis ;
Xue, Yongquan ;
Zezas, Andreas .
ASTROPHYSICAL JOURNAL, 2013, 762 (01)
[7]   The first release COSMOS optical and near-IR data and catalog [J].
Capak, P. ;
Aussel, H. ;
Ajiki, M. ;
McCracken, H. J. ;
Mobasher, B. ;
Scoville, N. ;
Shopbell, P. ;
Taniguchi, Y. ;
Thompson, D. ;
Tribiano, S. ;
Sasaki, S. ;
Blain, A. W. ;
Brusa, M. ;
Carilli, C. ;
Comastri, A. ;
Carollo, C. M. ;
Cassata, P. ;
Colbert, J. ;
Ellis, R. S. ;
Elvis, M. ;
Giavalisco, M. ;
Green, W. ;
Guzzo, L. ;
Hasinger, G. ;
Ilbert, O. ;
Impey, C. ;
Jahnke, K. ;
Kartaltepe, J. ;
Kneib, J.-P. ;
Koda, J. ;
Koekemoer, A. ;
Komiyama, Y. ;
Leauthaud, A. ;
Lefevre, O. ;
Lilly, S. ;
Liu, C. ;
Massey, R. ;
Miyazaki, S. ;
Murayama, T. ;
Nagao, T. ;
Peacock, J. A. ;
Pickles, A. ;
Porciani, C. ;
Renzini, A. ;
Rhodes, J. ;
Rich, M. ;
Salvato, M. ;
Sanders, D. B. ;
Scarlata, C. ;
Schiminovich, D. .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2007, 172 (01) :99-116
[8]   CHANDRA COUNTERPARTS OF CANDELS GOODS-S SOURCES [J].
Cappelluti, N. ;
Comastri, A. ;
Fontana, A. ;
Zamorani, G. ;
Amorin, R. ;
Castellano, M. ;
Merlin, E. ;
Santini, P. ;
Elbaz, D. ;
Schreiber, C. ;
Shu, X. ;
Wang, T. ;
Dunlop, J. S. ;
Bourne, N. ;
Bruce, V. A. ;
Buitrago, F. ;
Michalowski, Michal J. ;
Derriere, S. ;
Ferguson, H. C. ;
Faber, S. M. ;
Vito, F. .
ASTROPHYSICAL JOURNAL, 2016, 823 (02)
[9]   CROSS-CORRELATING COSMIC INFRARED AND X-RAY BACKGROUND FLUCTUATIONS: EVIDENCE OF SIGNIFICANT BLACK HOLE POPULATIONS AMONG THE CIB SOURCES [J].
Cappelluti, N. ;
Kashlinsky, A. ;
Arendt, R. G. ;
Comastri, A. ;
Fazio, G. G. ;
Finoguenov, A. ;
Hasinger, G. ;
Mather, J. C. ;
Miyaji, T. ;
Moseley, S. H. .
ASTROPHYSICAL JOURNAL, 2013, 769 (01)
[10]   The nature of the unresolved extragalactic cosmic soft X-ray background [J].
Cappelluti, N. ;
Ranalli, P. ;
Roncarelli, M. ;
Arevalo, P. ;
Zamorani, G. ;
Comastri, A. ;
Gilli, R. ;
Rovilos, E. ;
Vignali, C. ;
Allevato, V. ;
Finoguenov, A. ;
Miyaji, T. ;
Nicastro, F. ;
Georgantopoulos, I. ;
Kashlinsky, A. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2012, 427 (01) :651-663