BAT AGN Spectroscopic Survey. V. X-Ray Properties of the Swift/BAT 70-month AGN Catalog
CRC. RicciBTB. TrakhtenbrotMJM. J. KossYUY. UedaIDI. Del Vecchio
Indexed inarxivcrossrefdoaj
Abstract
Abstract 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 ( keV) with 70-month averaged Swift /BAT data. The nonblazar AGNs of our sample are almost equally divided into unobscured ( ) and obscured ( ) AGNs, and their Swift /BAT continuum is systematically steeper than the 0.3–10 keV emission,…
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Authors
21- CRC. RicciCorresponding
- BTB. Trakhtenbrot
- MJM. J. Koss
- YUY. Ueda
- IDI. Del Vecchio
Topics & keywords
Topics
Keywords
- Active galactic nucleus
- Accretion (finance)
- Cutoff
- Supermassive black hole
- Accretion disc
- Reflection (computer programming)
- Photon
- Galaxy
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Funding
- NSNational Science FoundationAwards: PP00P2_166159, PP00P2_138979, 1141218, 11473002
- NANational Aeronautics and Space AdministrationAward: 2016YFA0400702
- CICalifornia Institute of Technology
- CAChinese Academy of Sciences South America Center for Astronomy
- UOUniversity of Leicester
- ICImperial College London
- ECEuropean CommissionAward: 337595
- MOMinistry of Education, Culture, Sports, Science and Technology
- SNSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungAwards: PP00P2_138979, PZ00P2, 200021_157021, PP00P2_166159, 154799
- NNNational Natural Science Foundation of ChinaAwards: 11473002, 2016YFA0400702
- CAChinese Academy of SciencesAward: 2016YFA0400702
- JPJet Propulsion Laboratory
- GSGoddard Space Flight Center
- UOUniversity of California, Los Angeles
- SAScience and Technology Facilities CouncilAward: ST/J003697/2
- JSJapan Society for the Promotion of ScienceAward: 17K05384
- CNComisión Nacional de Investigación Científica y TecnológicaAwards: PFB-06, PFB-06/2007, 1160999, ACT1101, Basal-CATA PFB-06/2007