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.
| 元の言語 | 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 | |
| 出版物ステータス | Published - 2007 |
| イベント | 1st Gamma-ray Large Area Space Telescope Symposium, GLAST - Stanford, CA 継続期間: 2007 2 5 → 2007 2 8 |
Other
| Other | 1st Gamma-ray Large Area Space Telescope Symposium, GLAST |
|---|---|
| 市 | Stanford, CA |
| 期間 | 07/2/5 → 07/2/8 |
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ASJC Scopus subject areas
- Physics and Astronomy(all)
これを引用
Suzaku HXD-WAM observations of gamma-ray prompt emission and collaboration with GLAST. / 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.
AIP Conference Proceedings. 巻 921 2007. p. 106-108.研究成果: Conference contribution
}
TY - GEN
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
UR - http://www.scopus.com/inward/record.url?scp=77957868982&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=77957868982&partnerID=8YFLogxK
U2 - 10.1063/1.2757279
DO - 10.1063/1.2757279
M3 - Conference contribution
AN - SCOPUS:77957868982
SN - 9780735404311
VL - 921
SP - 106
EP - 108
BT - AIP Conference Proceedings
ER -