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.
Original language | English |
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Title of host publication | AIP Conference Proceedings |
Pages | 106-108 |
Number of pages | 3 |
Volume | 921 |
DOIs | |
Publication status | Published - 2007 |
Event | 1st Gamma-ray Large Area Space Telescope Symposium, GLAST - Stanford, CA Duration: 2007 Feb 5 → 2007 Feb 8 |
Other
Other | 1st Gamma-ray Large Area Space Telescope Symposium, GLAST |
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City | Stanford, CA |
Period | 07/2/5 → 07/2/8 |
Keywords
- Gamma-ray bursts
ASJC Scopus subject areas
- Physics and Astronomy(all)