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 | |
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)