BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog

被引：322

作者：

Ricci, C. ^{[1
,2
,3
,4
,5
]}

Trakhtenbrot, B. ^{[6
]}

Koss, M. J. ^{[6
]}

Ueda, Y. ^{[2
]}

Del Vecchio, I. ^{[7
]}

Treister, E. ^{[1
]}

Schawinski, K. ^{[6
]}

Paltani, S. ^{[8
]}

Oh, K. ^{[6
]}

Lamperti, I. ^{[6
]}

Berney, S. ^{[6
]}

Gandhi, P. ^{[9
]}

Ichikawa, K. ^{[10
,11
,12
]}

Bauer, F. E. ^{[1
,13
,14
]}

Ho, L. C. ^{[3
,15
]}

Asmus, D. ^{[16
]}

Beckmann, V. ^{[17
]}

Soldi, S. ^{[18
]}

Balokovic, M. ^{[19
]}

Gehrels, N. ^{[20
]}

Markwardt, C. B. ^{[21
,22
]}

机构：

[1] Pontificia Univ Catolica Chile, Fac Fis, Inst Astrofis, Casilla 306, Santiago 22, Chile

[2] Kyoto Univ, Dept Astron, Sakyo Ku, Oiwake Cho, Kyoto 6068502, Japan

[3] Peking Univ, Kavli Inst Astron & Astrophys, Beijing 100871, Peoples R China

[4] Chinese Acad Sci, South Amer Ctr Astron, Camino El Observ 1515, Santiago, Chile

[5] Chinese Acad Sci, China Chile Joint Ctr Astron, Camino El Observ 1515, Santiago, Chile

[6] ETH, Dept Phys, Inst Astron, Wolfgang Pauli Str 27, CH-8093 Zurich, Switzerland

[7] Univ Zagreb, Dept Phys, Bijenicka Cesta 32, HR-10002 Zagreb, Croatia

[8] Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland

[9] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England

[10] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[11] Univ Texas San Antonio, Dept Phys & Astron, One UTSA Circle, San Antonio, TX 78249 USA

[12] Columbia Univ, Dept Astron, 550 West 120th St, New York, NY 10027 USA

[13] Space Sci Inst, 4750 Walnut St,Suite 205, Boulder, CO 80301 USA

[14] Millenium Inst Astrophys, Santiago, Chile

[15] Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China

[16] European Southern Observ, Casilla 19001, Santiago 19, Chile

[17] CNRS, IN2P3, 3 Rue Michel Ange, F-75794 Paris 16, France

[18] Univ Paris Diderot, CNRS, IN2P3, Ctr Franois Arago,APC, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France

[19] CALTECH, Cahill Ctr Astron & Astrophys, Pasadena, CA 91125 USA

[20] NASA, Goddard Space Flight Ctr, Mail Code 661, Greenbelt, MD 20771 USA

[21] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[22] NASA, Goddard Space Flight Ctr, Astroparticle Phys Lab, Mail Code 661, Greenbelt, MD 20771 USA

来源：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2017年 / 233卷 / 02期

基金：

瑞士国家科学基金会; 美国国家科学基金会; 美国国家航空航天局;

关键词：

galaxies: active; galaxies: Seyfert; quasars: general; X-rays: diffuse background; X-rays: general; ACTIVE GALACTIC NUCLEI; SUPERMASSIVE BLACK-HOLES; BURST ALERT TELESCOPE; K-ALPHA LINE; SPECTRAL ENERGY-DISTRIBUTIONS; XMM-NEWTON OBSERVATIONS; STAR-FORMING GALAXIES; BROAD EMISSION-LINES; ULTRA-FAST OUTFLOWS; SEYFERT; GALAXIES;

D O I：

10.3847/1538-4365/aa96ad

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Hard X-ray (>= 10 keV) observations of active galactic nuclei (AGNs) can shed light on some of the most obscured episodes of accretion onto supermassive black holes. The 70-month Swift/BAT all-sky survey, which probes the 14-195 keV energy range, has currently detected 838 AGNs. We report here on the broadband X-ray (0.3-150 keV) characteristics of these AGNs, obtained by combining XMM-Newton, Swift/XRT, ASCA, Chandra, and Suzaku observations in the soft X-ray band (<= 10 keV) with 70-month averaged Swift/BAT data. The nonblazar AGNs of our sample are almost equally divided into unobscured (N-H < 10(22)cm(-2)) and obscured (N-H >= 10(22) cm(-2)) AGNs, and their Swift/BAT continuum is systematically steeper than the 0.3-10 keV emission, which suggests that the presence of a high-energy cutoff is almost ubiquitous. We discuss the main X-ray spectral parameters obtained, such as the photon index, the reflection parameter, the energy of the cutoff, neutral and ionized absorbers, and the soft excess for both obscured and unobscured AGNs.

引用

页数：38

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