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Suzaku/Fermi Challenges to Relativistic Jets in AGN
https://jaxa.repo.nii.ac.jp/records/4938
https://jaxa.repo.nii.ac.jp/records/4938e1790a23-ddad-4f68-a871-54a8666a7b34
名前 / ファイル | ライセンス | アクション |
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64574006.pdf (334.4 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/Fermi Challenges to Relativistic Jets in AGN | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | AGN: blazars, Fermi, Suzaku, Swift, multiwavelength monitoring | |||||
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 |
片岡, 淳
× 片岡, 淳× 佐藤, 理江× Kataoka, Jun× Sato, Rie. K.× Madejski, G. M.× Fermi-LAT, collaboration |
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著者所属 | ||||||
早稲田大学理工学術院総合研究所 | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究本部 | ||||||
著者所属(英) | ||||||
en | ||||||
Research Institute for Science and Engineering, Waseda University | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||
著者所属(英) | ||||||
en | ||||||
KIPAC/Stanford Linear Accelerator Center, Stanford University | ||||||
著者所属(英) | ||||||
en | ||||||
Fermi-LAT collaboration | ||||||
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. 22-25, 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 | In next five years, dramatic progress is anticipated for the AGN studies, as we have two important missions to observe celestial sources in the high energy regime: Fermi and Suzaku. Simultaneous monitoring observations by the two instruments (Fermi-LAT and Suzaku XIS/HXD) will be particularly valuable for variable radio-loud AGN, allowing the cross-correlations of time series as well as detailed modeling of the spectral evolution between the X-ray and gamma-ray energy bands. In this paper, we particularly focus on the results from recent Suzaku X-ray observations of five flat-spectrum radio quasars (FSRQs), simultaneously observed with Fermi. Our aim is to reveal the nature of high-energy emission of luminous blazars in their quiescent/low-activity states covering the frequency range from 10(exp 14) Hz up to 10(exp 25) Hz. | |||||
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: AA0064574006 | |||||
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 |