Detailed analyses of GRB 060105 X-ray afterglow observed by Suzaku

被引：0
|
作者：
Nakagawa, Y. E. [1 ]
Tashiro, M.
Abe, K.
Yoshida, A.
Yamaoka, K.
Nakazawa, K.
Murakami, T.
Yonetoku, D.
Kawai, N.
Nousek, J.
Ishikawa, N.
Urata, Y.
Onda, K.
Tamagawa, T.
Suzuki, M.
Kuwahara, M.
Takahashi, T.
Yamauchi, M.
Sonoda, E.
Maeno, S.
Kinugasa, K.
Kohmura, T.
Torii, K.
Ueda, Y.
Kubota, K.
Sugiyasu, K.
Kodaira, H.
Okuno, S.
Yoshinari, S.
Shimokawabe, T.
Ishimura, T.
Ricker, G. R.
Reeves, J. N.
Angelini, L.
Kaluzienski, L. J.
Kelley, R. L.
机构：
[1] Aoyama Gakuin Univ, Dept Math & Phys, Kanagawa, Japan
[2] Saitama Univ, High Energy Astrophys Lab, Saitama, Japan
[3] Inst Phys & Chem Res, Saitama, Japan
[4] ISAS JAXA, Sagamihara, Kanagawa, Japan
[5] Tokyo Inst Technol, Dept Phys, Tokyo 152, Japan
[6] Penn State Univ, University Pk, PA 16802 USA
[7] Miyazaki Univ, Fac Engn, Miyazaki 88921, Japan
[8] Gunma Astron Observ, Gunma, Japan
[9] Kogakuin Univ, Tokyo, Japan
[10] Osaka Univ, Osaka, Japan
[11] Kyoto Univ, Kyoto, Japan
[12] MIT, Ctr Space Res, Cambridge, MA 02139 USA
[13] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[14] Kanazawa Univ, Kanazawa, Ishikawa 920, Japan
来源：
NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS | 2006年 / 121卷 / 12期
关键词：
D O I：
10.1393/ncb/i2007-10316-8
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
GRB 060105 was detected with the BAT instrument on-board Swift. The Suzaku follow-up observation started just 5.3 hours after the trigger with the XIS and HXD instruments. The XIS detected an uncatalogued fading source and its position was consistent with that previously reported by Swift XRT. We performed the spectral analyses using the data derived from Suzaku XIS and Swift XRT, and found that the spectrum of X-ray afterglow was well reproduced by the absorbed power law model.
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页码：1531 / 1533
页数：3
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