Strategy of the Suzaku gamma-ray burst observations

M. S. Tashiro; K. Abe; L. Angelini; Y. Endo; T. Enoto; Y. Fukazawa; S. Hong; N. Ishikawa; L. J. Kaluzienski; N. Kawai; R. L. Kelley; K. Kinugasa; H. Kodaira; T. Kohmura; M. Kokubun; K. Kubota; S. Maeno; K. Makishima; R. Miyawaki; T. Murakami; Y. E. Nakagawa; K. Nakazawa; J. A. Nousek; M. Ohno; S. Okuno; K. Onda; J. N. Reeves; G. Ricker; G. Sato; E. Sonoda; S. Sugita; M. Suzuki; T. Takahashi; T. Takahashi; T. Tamagawa; Y. Terada; K. Torii; Y. Ueda; Y. Urata; K. Yamaoka; M. Yamauchi; A. Yoshida; S. Yoshinari; D. Yonetoku

doi:10.1016/j.asr.2007.02.081

Strategy of the Suzaku gamma-ray burst observations

M. S. Tashiro^*, K. Abe, L. Angelini, Y. Endo, T. Enoto, Y. Fukazawa, S. Hong, N. Ishikawa, L. J. Kaluzienski, N. Kawai, R. L. Kelley, K. Kinugasa, H. Kodaira, T. Kohmura, M. Kokubun, K. Kubota, S. Maeno, K. Makishima, R. Miyawaki, T. MurakamiY. E. Nakagawa, K. Nakazawa, J. A. Nousek, M. Ohno, S. Okuno, K. Onda, J. N. Reeves, G. Ricker, G. Sato, E. Sonoda, S. Sugita, M. Suzuki, T. Takahashi, T. Takahashi, T. Tamagawa, Y. Terada, K. Torii, Y. Ueda, Y. Urata, K. Yamaoka, M. Yamauchi, A. Yoshida, S. Yoshinari, D. Yonetoku

^*この研究の対応する著者

理工学術院総合研究所

研究成果: Article › 査読

1 被引用数 (Scopus)

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Suzaku launched in July 2005 is equipped with the wideband instruments covering 0.3-700 keV. In addition to these main instruments, active shield counters of the hard X-ray detector are designed to be a wideband all-sky monitor (WAM). The WAM is a powerful gamma-ray burst monitor with a wide energy range of 50-5000 keV and with a large effective area of 400 cm² even around 1 MeV. The paper describes the strategy for the prompt GRB observation with the WAM, and the follow-up observation of X-ray afterglows with the narrow field instruments. So far, the WAM has detected 53 GRBs and half of them were detected simultaneously with other satellites. In addition to that, from at least 8 GRBs, including a bright and hard GRB 051008, it is succeeded to observe significant gamma-ray emission up to 1 MeV. The X-ray afterglow observations were carried out on January 5 and on September 4, 2006. Their results are reported in separate paper.

本文言語	English
ページ（範囲）	1255-1258
ページ数	4
ジャーナル	Advances in Space Research
巻	40
号	8
DOI	https://doi.org/10.1016/j.asr.2007.02.081
出版ステータス	Published - 2007

ASJC Scopus subject areas

宇宙惑星科学
天文学と天体物理学

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10.1016/j.asr.2007.02.081

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Tashiro, M. S., Abe, K., Angelini, L., Endo, Y., Enoto, T., Fukazawa, Y., Hong, S., Ishikawa, N., Kaluzienski, L. J., Kawai, N., Kelley, R. L., Kinugasa, K., Kodaira, H., Kohmura, T., Kokubun, M., Kubota, K., Maeno, S., Makishima, K., Miyawaki, R., ... Yonetoku, D. (2007). Strategy of the Suzaku gamma-ray burst observations. Advances in Space Research, 40(8), 1255-1258. https://doi.org/10.1016/j.asr.2007.02.081

Tashiro, MS, Abe, K, Angelini, L, Endo, Y, Enoto, T, Fukazawa, Y, Hong, S, Ishikawa, N, Kaluzienski, LJ, Kawai, N, Kelley, RL, Kinugasa, K, Kodaira, H, Kohmura, T, Kokubun, M, Kubota, K, Maeno, S, Makishima, K, Miyawaki, R, Murakami, T, Nakagawa, YE, Nakazawa, K, Nousek, JA, Ohno, M, Okuno, S, Onda, K, Reeves, JN, Ricker, G, Sato, G, Sonoda, E, Sugita, S, Suzuki, M, Takahashi, T, Takahashi, T, Tamagawa, T, Terada, Y, Torii, K, Ueda, Y, Urata, Y, Yamaoka, K, Yamauchi, M, Yoshida, A, Yoshinari, S & Yonetoku, D 2007, 'Strategy of the Suzaku gamma-ray burst observations', Advances in Space Research, vol. 40, no. 8, pp. 1255-1258. https://doi.org/10.1016/j.asr.2007.02.081

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title = "Strategy of the Suzaku gamma-ray burst observations",

abstract = "Suzaku launched in July 2005 is equipped with the wideband instruments covering 0.3-700 keV. In addition to these main instruments, active shield counters of the hard X-ray detector are designed to be a wideband all-sky monitor (WAM). The WAM is a powerful gamma-ray burst monitor with a wide energy range of 50-5000 keV and with a large effective area of 400 cm2 even around 1 MeV. The paper describes the strategy for the prompt GRB observation with the WAM, and the follow-up observation of X-ray afterglows with the narrow field instruments. So far, the WAM has detected 53 GRBs and half of them were detected simultaneously with other satellites. In addition to that, from at least 8 GRBs, including a bright and hard GRB 051008, it is succeeded to observe significant gamma-ray emission up to 1 MeV. The X-ray afterglow observations were carried out on January 5 and on September 4, 2006. Their results are reported in separate paper.",

keywords = "Gamma-ray burst, Strategy, Suzaku, Swift, X-ray observation",

author = "Tashiro, {M. S.} and K. Abe and L. Angelini and Y. Endo and T. Enoto and Y. Fukazawa and S. Hong and N. Ishikawa and Kaluzienski, {L. J.} and N. Kawai and Kelley, {R. L.} and K. Kinugasa and H. Kodaira and T. Kohmura and M. Kokubun and K. Kubota and S. Maeno and K. Makishima and R. Miyawaki and T. Murakami and Nakagawa, {Y. E.} and K. Nakazawa and Nousek, {J. A.} and M. Ohno and S. Okuno and K. Onda and Reeves, {J. N.} and G. Ricker and G. Sato and E. Sonoda and S. Sugita and M. Suzuki and T. Takahashi and T. Takahashi and T. Tamagawa and Y. Terada and K. Torii and Y. Ueda and Y. Urata and K. Yamaoka and M. Yamauchi and A. Yoshida and S. Yoshinari and D. Yonetoku",

year = "2007",

doi = "10.1016/j.asr.2007.02.081",

language = "English",

volume = "40",

pages = "1255--1258",

journal = "Advances in Space Research",

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TY - JOUR

T1 - Strategy of the Suzaku gamma-ray burst observations

AU - Tashiro, M. S.

AU - Abe, K.

AU - Angelini, L.

AU - Endo, Y.

AU - Enoto, T.

AU - Fukazawa, Y.

AU - Hong, S.

AU - Ishikawa, N.

AU - Kaluzienski, L. J.

AU - Kawai, N.

AU - Kelley, R. L.

AU - Kinugasa, K.

AU - Kodaira, H.

AU - Kohmura, T.

AU - Kokubun, M.

AU - Kubota, K.

AU - Maeno, S.

AU - Makishima, K.

AU - Miyawaki, R.

AU - Murakami, T.

AU - Nakagawa, Y. E.

AU - Nakazawa, K.

AU - Nousek, J. A.

AU - Ohno, M.

AU - Okuno, S.

AU - Onda, K.

AU - Reeves, J. N.

AU - Ricker, G.

AU - Sato, G.

AU - Sonoda, E.

AU - Sugita, S.

AU - Suzuki, M.

AU - Takahashi, T.

AU - Tamagawa, T.

AU - Terada, Y.

AU - Torii, K.

AU - Ueda, Y.

AU - Urata, Y.

AU - Yamaoka, K.

AU - Yamauchi, M.

AU - Yoshida, A.

AU - Yoshinari, S.

AU - Yonetoku, D.

PY - 2007

Y1 - 2007

N2 - Suzaku launched in July 2005 is equipped with the wideband instruments covering 0.3-700 keV. In addition to these main instruments, active shield counters of the hard X-ray detector are designed to be a wideband all-sky monitor (WAM). The WAM is a powerful gamma-ray burst monitor with a wide energy range of 50-5000 keV and with a large effective area of 400 cm2 even around 1 MeV. The paper describes the strategy for the prompt GRB observation with the WAM, and the follow-up observation of X-ray afterglows with the narrow field instruments. So far, the WAM has detected 53 GRBs and half of them were detected simultaneously with other satellites. In addition to that, from at least 8 GRBs, including a bright and hard GRB 051008, it is succeeded to observe significant gamma-ray emission up to 1 MeV. The X-ray afterglow observations were carried out on January 5 and on September 4, 2006. Their results are reported in separate paper.

AB - Suzaku launched in July 2005 is equipped with the wideband instruments covering 0.3-700 keV. In addition to these main instruments, active shield counters of the hard X-ray detector are designed to be a wideband all-sky monitor (WAM). The WAM is a powerful gamma-ray burst monitor with a wide energy range of 50-5000 keV and with a large effective area of 400 cm2 even around 1 MeV. The paper describes the strategy for the prompt GRB observation with the WAM, and the follow-up observation of X-ray afterglows with the narrow field instruments. So far, the WAM has detected 53 GRBs and half of them were detected simultaneously with other satellites. In addition to that, from at least 8 GRBs, including a bright and hard GRB 051008, it is succeeded to observe significant gamma-ray emission up to 1 MeV. The X-ray afterglow observations were carried out on January 5 and on September 4, 2006. Their results are reported in separate paper.

KW - Gamma-ray burst

KW - Strategy

KW - Suzaku

KW - Swift

KW - X-ray observation

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U2 - 10.1016/j.asr.2007.02.081

DO - 10.1016/j.asr.2007.02.081

M3 - Article

AN - SCOPUS:35548988933

SN - 0273-1177

VL - 40

SP - 1255

EP - 1258

JO - Advances in Space Research

JF - Advances in Space Research

IS - 8

ER -

Strategy of the Suzaku gamma-ray burst observations

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