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Suzaku Wide-band All-sky Monitor observations of GRB prompt emissions

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.2207890· OSTI ID:20798682
;  [1]; ; ;  [2];  [3]; ; ; ;  [4];  [4]; ; ;  [5];  [5]; ; ;  [6]
  1. Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 229-8558 (Japan)
  2. Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 (Japan)
  3. RIKEN, 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan)
  4. Saitama University, 255 Shimo-Ohkubo, Saitama-city, Saitama 338-8570 (Japan)
  5. University of Tokyo, 1-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan)
  6. ISAS/JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510 (Japan)
The Suzaku Wide-band All-sky Monitor (WAM), realized by large thick anti-coincidence shields of the Hard X-ray Detector (HXD), can be powerful gamma-ray burst (GRB) detector which is sensitive to 50-5000 keV gamma-rays. The WAM is now in a full operational phase, and we have already detected some GRBs simultaneously with other satellites (Swift, Konus-Wind, HETE2 and INTEGRAL SPI/ACS). The most impressive event among detected GRBs is GRB051008, which was detected up to 2 MeV with the WAM. In this paper, we report on the WAM in-flight performance as a GRB monitor from initial three-months operations, focusing on the GRB trigger status and spectral analysis of GRB051008 and GRB051111 combined with Swift.
OSTI ID:
20798682
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 836; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English

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