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Suzaku Observation of Six New Swift/BAT AGNs: Evidence for Two Types of Obscured Population
https://jaxa.repo.nii.ac.jp/records/5072
https://jaxa.repo.nii.ac.jp/records/50725b88c6ed-2f74-4669-85db-5d571a8fc6b1
名前 / ファイル | ライセンス | アクション |
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64574140.pdf (219.5 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Suzaku Observation of Six New Swift/BAT AGNs: Evidence for Two Types of Obscured Population | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: active - gamma rays: observations - X-rays: galaxies - X-rays: general | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
著者 |
江口, 智士
× 江口, 智士× 上田, 佳宏× 寺島, 雄一× Eguchi, Satoshi× Ueda, Yoshihiro× Terashima, Yuichi× Mushotzky, Richard× Tueller, Jack |
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著者所属 | ||||||
京都大学理学研究科宇宙物理学教室 | ||||||
著者所属 | ||||||
京都大学理学研究科宇宙物理学教室 | ||||||
著者所属 | ||||||
愛媛大学理学部物理学科 | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Astronomy, Kyoto University | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Phyisics, Faculty of Science, Ehime University | ||||||
著者所属(英) | ||||||
en | ||||||
NASA/Goddard Space Flight Center | ||||||
著者所属(英) | ||||||
en | ||||||
NASA/Goddard Space Flight Center | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構 | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料: en : JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H 巻 JAXA-SP-09-008E, p. 368-369, 発行日 2010-02-26 |
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会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We present a systematic spectral analysis with Suzaku of six AGNs detected in the Swift/BAT hard X-ray (15 - 200 keV) survey. The 0.5 - 200 keV spectra of these sources can be uniformly fit with a base model consisting of heavily absorbed (logN(sub H) > 23.5 cm(sup -2)) transmitted components, scattered lights, a reflection component, and an iron-K emission line. There are two distinct groups, three "new type" AGNs (including the two sources reported by Ueda et al. 2007) with an extremely small scattered fraction (f(sub scat) < 0.5 % ) and strong reflection component (R = Omega/2pi greater than or approximately equal to 0.8, where Omega is the solid angle of the reflector), and three "classical type" ones with f(sub scat) > 0.5 % and R greater than or approximately equal to 0.8. The spectral parameters suggest that the new type has an optically thick torus for Thomson scattering (N(sub H) approximately 10(sup 25) cm(sup -2)) with a small opening angle of theta approximately 20 deg viewed in a rather face-on geometry, while the classical type has a thin torus (logN(sub H) approximately 23 - 24 cm(sup -2)) with theta > or similar to 30 deg. We infer that a significant number of new type AGNs with an edge-on view is missing in the current all-sky hard X-ray surveys. | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1349-113X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11984031 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064574140 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-09-008E |