Suzaku HXD-WAM observations of gamma-ray prompt emission and collaboration with GLAST

Y. Fukazawa; M. Ohno; T. Takahashi; T. Asano; T. Uehara; K. Yamaoka; S. Sugita; Y. Terada; T. Tamagawa; M. Suzuki; M. Tashiro; Y. Urata; K. Abe; K. Onda; M. Suzuki; E. Sonoda; G. Sato; T. Enoto; K. Makishima; T. Takahashi; M. Kokubun; K. Nakazawa

doi:10.1063/1.2757279

Suzaku HXD-WAM observations of gamma-ray prompt emission and collaboration with GLAST

Y. Fukazawa^*, M. Ohno, T. Takahashi, T. Asano, T. Uehara, K. Yamaoka, S. Sugita, Y. Terada, T. Tamagawa, M. Suzuki, M. Tashiro, Y. Urata, K. Abe, K. Onda, M. Suzuki, E. Sonoda, G. Sato, T. Enoto, K. Makishima, T. TakahashiM. Kokubun, K. Nakazawa

^*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: Conference contribution

1 被引用数 (Scopus)

抄録

The wide-band all-sky monitor (WAM) onboard Suzaku has the largest effective area in 300-5000 keV, and thus very powerful to constrain the E peak and high energy tail of gamma-ray burst prompt emission. Collaboration with GLAST will give us high-quality data of gamma-ray prompt emissions to probe and resolve the emission mechanism and central engine of gamma-ray bursts. Here we report initial results of the WAM and address on the collaboration with GLAST.

本文言語	English
ホスト出版物のタイトル	AIP Conference Proceedings
ページ	106-108
ページ数	3
巻	921
DOI	https://doi.org/10.1063/1.2757279
出版ステータス	Published - 2007
イベント	1st Gamma-ray Large Area Space Telescope Symposium, GLAST - Stanford, CA 継続期間: 2007 2月 5 → 2007 2月 8

Other

Other	1st Gamma-ray Large Area Space Telescope Symposium, GLAST
City	Stanford, CA
Period	07/2/5 → 07/2/8

ASJC Scopus subject areas

物理学および天文学（全般）

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10.1063/1.2757279

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引用スタイル

Fukazawa, Y., Ohno, M., Takahashi, T., Asano, T., Uehara, T., Yamaoka, K., Sugita, S., Terada, Y., Tamagawa, T., Suzuki, M., Tashiro, M., Urata, Y., Abe, K., Onda, K., Suzuki, M., Sonoda, E., Sato, G., Enoto, T., Makishima, K., ... Nakazawa, K. (2007). Suzaku HXD-WAM observations of gamma-ray prompt emission and collaboration with GLAST. In AIP Conference Proceedings (Vol. 921, pp. 106-108) https://doi.org/10.1063/1.2757279

Fukazawa, Y, Ohno, M, Takahashi, T, Asano, T, Uehara, T, Yamaoka, K, Sugita, S, Terada, Y, Tamagawa, T, Suzuki, M, Tashiro, M, Urata, Y, Abe, K, Onda, K, Suzuki, M, Sonoda, E, Sato, G, Enoto, T, Makishima, K, Takahashi, T, Kokubun, M & Nakazawa, K 2007, Suzaku HXD-WAM observations of gamma-ray prompt emission and collaboration with GLAST. in AIP Conference Proceedings. vol. 921, pp. 106-108, 1st Gamma-ray Large Area Space Telescope Symposium, GLAST, Stanford, CA, 07/2/5. https://doi.org/10.1063/1.2757279

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title = "Suzaku HXD-WAM observations of gamma-ray prompt emission and collaboration with GLAST",

abstract = "The wide-band all-sky monitor (WAM) onboard Suzaku has the largest effective area in 300-5000 keV, and thus very powerful to constrain the E peak and high energy tail of gamma-ray burst prompt emission. Collaboration with GLAST will give us high-quality data of gamma-ray prompt emissions to probe and resolve the emission mechanism and central engine of gamma-ray bursts. Here we report initial results of the WAM and address on the collaboration with GLAST.",

keywords = "Gamma-ray bursts",

author = "Y. Fukazawa and M. Ohno and T. Takahashi and T. Asano and T. Uehara and K. Yamaoka and S. Sugita and Y. Terada and T. Tamagawa and M. Suzuki and M. Tashiro and Y. Urata and K. Abe and K. Onda and M. Suzuki and E. Sonoda and G. Sato and T. Enoto and K. Makishima and T. Takahashi and M. Kokubun and K. Nakazawa",

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doi = "10.1063/1.2757279",

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T1 - Suzaku HXD-WAM observations of gamma-ray prompt emission and collaboration with GLAST

AU - Fukazawa, Y.

AU - Ohno, M.

AU - Takahashi, T.

AU - Asano, T.

AU - Uehara, T.

AU - Yamaoka, K.

AU - Sugita, S.

AU - Terada, Y.

AU - Tamagawa, T.

AU - Suzuki, M.

AU - Tashiro, M.

AU - Urata, Y.

AU - Abe, K.

AU - Onda, K.

AU - Suzuki, M.

AU - Sonoda, E.

AU - Sato, G.

AU - Enoto, T.

AU - Makishima, K.

AU - Takahashi, T.

AU - Kokubun, M.

AU - Nakazawa, K.

PY - 2007

Y1 - 2007

N2 - The wide-band all-sky monitor (WAM) onboard Suzaku has the largest effective area in 300-5000 keV, and thus very powerful to constrain the E peak and high energy tail of gamma-ray burst prompt emission. Collaboration with GLAST will give us high-quality data of gamma-ray prompt emissions to probe and resolve the emission mechanism and central engine of gamma-ray bursts. Here we report initial results of the WAM and address on the collaboration with GLAST.

AB - The wide-band all-sky monitor (WAM) onboard Suzaku has the largest effective area in 300-5000 keV, and thus very powerful to constrain the E peak and high energy tail of gamma-ray burst prompt emission. Collaboration with GLAST will give us high-quality data of gamma-ray prompt emissions to probe and resolve the emission mechanism and central engine of gamma-ray bursts. Here we report initial results of the WAM and address on the collaboration with GLAST.

KW - Gamma-ray bursts

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U2 - 10.1063/1.2757279

DO - 10.1063/1.2757279

M3 - Conference contribution

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VL - 921

SP - 106

EP - 108

BT - AIP Conference Proceedings

T2 - 1st Gamma-ray Large Area Space Telescope Symposium, GLAST

Y2 - 5 February 2007 through 8 February 2007

ER -

Suzaku HXD-WAM observations of gamma-ray prompt emission and collaboration with GLAST

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