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Highly Ionized Warm Absorbers in AGNs: Simulations with the IXO Calorimeter
https://jaxa.repo.nii.ac.jp/records/5065
https://jaxa.repo.nii.ac.jp/records/5065d43b78aa-a4cd-4da0-8b38-5aa37e31fb53
名前 / ファイル | ライセンス | アクション |
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64574133.pdf (468.0 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 | Highly Ionized Warm Absorbers in AGNs: Simulations with the IXO Calorimeter | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | X-ray spectroscopy - absorption lines - AGNs | |||||
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 |
Tombesi, Francesco
× Tombesi, Francesco× Cappi, M.× Yaqoob, T.× Reeves, J.× Palumbo, G.G.C. |
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著者所属(英) | ||||||
en | ||||||
Dipartimento di Astronomia, Universita di Bologna | ||||||
著者所属(英) | ||||||
en | ||||||
INAF-IASF Bologna | ||||||
著者所属(英) | ||||||
en | ||||||
Department of Physics and Astronomy, Johns Hopkins University | ||||||
著者所属(英) | ||||||
en | ||||||
Astrophysics Group, School of Physical & Geographical Sciences, Keele University | ||||||
著者所属(英) | ||||||
en | ||||||
Dipartimento di Astronomia, Universita di Bologna | ||||||
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. 340-341, 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 have performed several simulations in order to test the scientific capabilities of the IXO calorimeter, with particular emphasis on the detection of absorption lines in the 3 - 11 keV band. We derived the flux limits for their detection on several time-scales, compared different response matrices available and simulated realistic spectra from photo-ionized warm absorbers in AGNs. This study illustrates the considerable improvements that this instrument will bring to high resolution spectroscopy, especially related to the study of accretion and outflows in the central regions of AGNs. | |||||
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: AA0064574133 | |||||
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 |