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Swift and Suzaku observations of the X-ray afterglow from the GRB 060105
https://sucra.repo.nii.ac.jp/records/13053
https://sucra.repo.nii.ac.jp/records/13053270be1f1-72b1-4145-a279-68c2616c7248
名前 / ファイル | ライセンス | アクション |
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A1002397.pdf (519.6 kB)
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2008-01-21 | |||||
タイトル | ||||||
タイトル | Swift and Suzaku observations of the X-ray afterglow from the GRB 060105 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | gamma rays : burst | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | radiation mechanisms : non-thermal | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | relativistic jet | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | X-rays : individual (GRB 060105) | |||||
キーワード | ||||||
主題Scheme | Other | |||||
主題 | X-rays : stars acceleration of particles | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
著者 |
田代, 信
× 田代, 信 |
|||||
著者 ローマ字 | ||||||
Tashiro, Makoto S. | ||||||
著者 ローマ字 | ||||||
Abe, Keiichi | ||||||
著者 ローマ字 | ||||||
Angelini, Lorella | ||||||
著者 ローマ字 | ||||||
Barthelmy, Scott | ||||||
著者 ローマ字 | ||||||
Gehrels, Neil | ||||||
著者 ローマ字 | ||||||
Ishikawa, Nobuyuki | ||||||
著者 ローマ字 | ||||||
Kaluzienski, Louis J. | ||||||
著者 ローマ字 | ||||||
Kawai, Nobuyuki | ||||||
著者 ローマ字 | ||||||
Kelley, Richard L. | ||||||
著者 ローマ字 | ||||||
Kinugasa, Kenzo | ||||||
著者 ローマ字 | ||||||
Kodaira, Hironobu | ||||||
著者 ローマ字 | ||||||
Kohmura, Takayoshi | ||||||
著者 ローマ字 | ||||||
Kubota, Kaori | ||||||
著者 ローマ字 | ||||||
Maeda, Yoshitomo | ||||||
著者 ローマ字 | ||||||
Maeno, Shouta | ||||||
著者 ローマ字 | ||||||
Murakami, Hiroshi | ||||||
著者 ローマ字 | ||||||
Murakami, Toshio | ||||||
著者 ローマ字 | ||||||
Nakagawa, Yujin E. | ||||||
著者 ローマ字 | ||||||
Nakazawa, Kazuhiro | ||||||
著者 ローマ字 | ||||||
Nousek, John | ||||||
著者 ローマ字 | ||||||
Okuno, Shin'ya | ||||||
著者 ローマ字 | ||||||
Onda, Kaori | ||||||
著者 ローマ字 | ||||||
Reeves, James N. | ||||||
著者 ローマ字 | ||||||
Ricker, George | ||||||
著者 ローマ字 | ||||||
Sato, Goro | ||||||
著者 ローマ字 | ||||||
Sonoda, Eri | ||||||
著者 ローマ字 | ||||||
Suzuki, Motoko | ||||||
著者 ローマ字 | ||||||
Takahashi, Tadayuki | ||||||
著者 ローマ字 | ||||||
Tamagawa, Toru | ||||||
著者 ローマ字 | ||||||
Torii, Ken'ichi | ||||||
著者 ローマ字 | ||||||
Ueda, Yoshihiro | ||||||
著者 ローマ字 | ||||||
Urata, Yuji | ||||||
著者 ローマ字 | ||||||
Yamaoka, Kazutaka | ||||||
著者 ローマ字 | ||||||
Yamauchi, Makoto | ||||||
著者 ローマ字 | ||||||
Yonetoku, Daisuke | ||||||
著者 ローマ字 | ||||||
Yoshida, Atsumasa | ||||||
著者 ローマ字 | ||||||
Yoshinari, Satoru | ||||||
著者 所属 | ||||||
埼玉大学大学院理工学研究科物質科学部門 | ||||||
著者 所属(別言語) | ||||||
Graduate School of Science and Engineering, Saitama University | ||||||
書誌情報 |
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 巻 59, p. S361-S367, 発行日 2007 |
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年月次 | ||||||
2007 | ||||||
出版者名 | ||||||
出版者 | Astronomical Society of Japan | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 00046264 | |||||
抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Results are presented of early X-ray afterglow observations of GRB 060105 by Swift and Suzaku. The bright, long gamma-ray burst GRB; 060105 triggered the Swift Burst Alert Telescope at 06:49:28 on 2006 January 5 (T-0). The Suzaku team commenced a pre-planned target of opportunity observation at 19 ks (5.3 hr) after the Swift trigger. The X-ray flux faded during observations from 6.8 x 10(-9) ergs(-1) cm(-2) (at T-0 + 87 s with the Swift/XRT) to 1.5 x 10(-13) erg s(-1) cm(-2) [at T-0 + 94-101 ks with the Suzaku X-ray Imaging Spectrometer (XIS)] in the 2-10 keV energy band. Following prompt emission and successive very steep decay, a shallow decay was observed from To + 187 s to T-0 + 1287 s. After an observation gap during T-0 + (1.5-3) ks, an extremely early steep decay was observed in T-0 + (4-30) ks. The lightcurve flattened again at T-0 + 30ks, and another steep decay followed from T-0 + 50ks to the end of observations. Both steep decays exhibited decay indices of 2.3-2.4. This very early break, if it is a jet break, is the earliest case among X-ray afterglow observations, suggesting a very narrow jet whose opening angle is well below 1 degrees. The unique Suzaku/XIS data allow us to set very tight upper limits on line emission or absorption in this GRB. For the reported pseudo-redshift of z = 4.0 +/- 1.3 the upper limit on the iron line equivalent width is 50 eV. | |||||
版 | ||||||
[著者版] | ||||||
著者版フラグ | ||||||
出版タイプ | AM | |||||
出版タイプResource | http://purl.org/coar/version/c_ab4af688f83e57aa | |||||
資源タイプ | ||||||
内容記述タイプ | Other | |||||
内容記述 | text | |||||
フォーマット | ||||||
内容記述タイプ | Other | |||||
内容記述 | application/pdf | |||||
作成日 | ||||||
日付 | 2008-01-21 | |||||
日付タイプ | Created | |||||
アイテムID | ||||||
A1002397 |