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Multiwavelengh simultaneous observation of Blazar 3C454.3 at the gamma rays flare in November 2007
https://jaxa.repo.nii.ac.jp/records/5281
https://jaxa.repo.nii.ac.jp/records/5281a0c7be7b-aa97-441d-bdf7-ce1f4b70f97f
名前 / ファイル | ライセンス | アクション |
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64306042.pdf (1.1 MB)
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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 | Multiwavelengh simultaneous observation of Blazar 3C454.3 at the gamma rays flare in November 2007 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | quasars : individual : 3C 454.3 - X rays : Suzaku - optical : MITSuME | |||||
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× 河合, 誠之× Mori, Y. A.× Kataoka, Jun× Kawai, Nobuyuki |
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著者所属 | ||||||
東京工業大学 | ||||||
著者所属 | ||||||
東京工業大学 | ||||||
著者所属 | ||||||
東京工業大学 | ||||||
著者所属(英) | ||||||
en | ||||||
Tokyo Institute of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Tokyo Institute of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
Tokyo Institute of Technology | ||||||
著者所属(英) | ||||||
en | ||||||
MiTSuME/Suzaku/AGILE Team | ||||||
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: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop 巻 JAXA-SP-08-014E, p. 212-216, 発行日 2009-02-27 |
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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 | Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008) | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The spectrum of blazars span over 20 decades from radio to gamma rays. To clarify a variety of physical phenomena of the blazar jets, a blazar must be monitored in multiwavelengths and simultaneously. We succeeded in simultaneous multiwavelength observation of a blazar 3C 454.3, a QHB (quasar-hosted blazar) at z = 0.859. It also belongs to the brightest quasar class, with its luminosity reaching 10(exp 48) erg/s. A huge gamma-ray flare of 3C 454.3 was reported by the AGILE satellite on November 2nd through December 1st, 2007. We proposed a ToO observation with the Suzaku satellite, which was approved and performed on Dec 5, 6. At the same time, we were monitoring its optical magnitudes in three colors (g', Rc, Ic) using the MITSuME Telescope at the ICRR Akeno Observatory, Yamanashi, Japan. Its R band magnitude increased from R=16 up to R=13.4 on December 1. We present the spectral energy distribution based on this multiwavelength observation, and discuss the emission models. | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
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: AA0064306042 | |||||
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-08-014E |