Spectrum feature of the underlying soft component of GRB041006.

Y. Shirasaki; A. Yoshida; N. Kawai; Y. Nakagawa; T. Tamagawa; M. Suzuki; S. Sugita; I. Takahashi; M. Arimoto; T. Shimokawabe; N. Vasquez; T. Ishimura; R. Sato; T. Sakamoto; M. Kuwahara; M. Matsuoka

doi:10.1063/1.2943433

Spectrum feature of the underlying soft component of GRB041006.

Y. Shirasaki, A. Yoshida, N. Kawai, Y. Nakagawa, T. Tamagawa, M. Suzuki, S. Sugita, I. Takahashi, M. Arimoto, T. Shimokawabe, N. Vasquez, T. Ishimura, R. Sato, T. Sakamoto, M. Kuwahara, M. Matsuoka

研究成果: Conference contribution

抄録

GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. The GRB shows a soft X-ray emission, a precursor before the onset of the main GRB, and also shows a soft X-ray tail after the end of the main peak. The light curves within four different energy bands show different features; At higher energy bands several peaks are seen in the light curve, while at lower energy band a single broader bump is dominated. It is expected that these different features are the result of mixture of several components each of which has different energetics and variability. To reveal the nature of each component, we analysed the time resolved spectra and they are successfully resolved into several components.

本文言語	English
ホスト出版物のタイトル	Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference
ページ	158-161
ページ数	4
巻	1000
DOI	https://doi.org/10.1063/1.2943433
出版ステータス	Published - 2008
外部発表	はい
イベント	Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007 - Santa Fe, NM 継続期間: 2007 11 5 → 2007 11 9

Other

Other	Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007
City	Santa Fe, NM
Period	07/11/5 → 07/11/9

ASJC Scopus subject areas

Physics and Astronomy(all)

文献へのアクセス

10.1063/1.2943433

フィンガープリント「Spectrum feature of the underlying soft component of GRB041006.」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル

Shirasaki, Y., Yoshida, A., Kawai, N., Nakagawa, Y., Tamagawa, T., Suzuki, M., Sugita, S., Takahashi, I., Arimoto, M., Shimokawabe, T., Vasquez, N., Ishimura, T., Sato, R., Sakamoto, T., Kuwahara, M., & Matsuoka, M. (2008). Spectrum feature of the underlying soft component of GRB041006. In Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference (Vol. 1000, pp. 158-161) https://doi.org/10.1063/1.2943433

Spectrum feature of the underlying soft component of GRB041006. / Shirasaki, Y.; Yoshida, A.; Kawai, N.; Nakagawa, Y.; Tamagawa, T.; Suzuki, M.; Sugita, S.; Takahashi, I.; Arimoto, M.; Shimokawabe, T.; Vasquez, N.; Ishimura, T.; Sato, R.; Sakamoto, T.; Kuwahara, M.; Matsuoka, M.

Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. Vol. 1000 2008. p. 158-161.

研究成果: Conference contribution

Shirasaki, Y, Yoshida, A, Kawai, N, Nakagawa, Y, Tamagawa, T, Suzuki, M, Sugita, S, Takahashi, I, Arimoto, M, Shimokawabe, T, Vasquez, N, Ishimura, T, Sato, R, Sakamoto, T, Kuwahara, M & Matsuoka, M 2008, Spectrum feature of the underlying soft component of GRB041006. in Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. vol. 1000, pp. 158-161, Santa Fe Conference on Gamma-Ray Bursts 2007, GRB 2007, Santa Fe, NM, 07/11/5. https://doi.org/10.1063/1.2943433

Shirasaki, Y. ; Yoshida, A. ; Kawai, N. ; Nakagawa, Y. ; Tamagawa, T. ; Suzuki, M. ; Sugita, S. ; Takahashi, I. ; Arimoto, M. ; Shimokawabe, T. ; Vasquez, N. ; Ishimura, T. ; Sato, R. ; Sakamoto, T. ; Kuwahara, M. ; Matsuoka, M. / Spectrum feature of the underlying soft component of GRB041006. Gamma-Ray Bursts 2007 - Proceedings of the Santa Fe Conference. Vol. 1000 2008. pp. 158-161

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AU - Yoshida, A.

AU - Kawai, N.

AU - Nakagawa, Y.

AU - Tamagawa, T.

AU - Suzuki, M.

AU - Sugita, S.

AU - Takahashi, I.

AU - Arimoto, M.

AU - Shimokawabe, T.

AU - Vasquez, N.

AU - Ishimura, T.

AU - Sato, R.

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AB - GRB 041006 was detected by HETE-2 at 12:18:08 UT on 06 October 2004. The GRB shows a soft X-ray emission, a precursor before the onset of the main GRB, and also shows a soft X-ray tail after the end of the main peak. The light curves within four different energy bands show different features; At higher energy bands several peaks are seen in the light curve, while at lower energy band a single broader bump is dominated. It is expected that these different features are the result of mixture of several components each of which has different energetics and variability. To reveal the nature of each component, we analysed the time resolved spectra and they are successfully resolved into several components.

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