GRB 190531B: CALET Gamma-Ray Burst Monitor detection
文献类型：GCN
| 作者 | Shimizu, Y; Yoshida, A; Sakamoto, T; Pal'Shin, V; Sugita, S; Kawakubo, Y; Yamaoka, K; Nakahira, S; Asaoka, Y; Ozawa, S |
| 发表日期 | 2019-06-04 |
| 出处 | GRB Coordinates Network |
| 英文摘要 | The long GRB 190531B (Fermi-LAT detection: Axelsson et al.,GCN Circ. 24701; Fermi-GBM observations: Veres and Meegan, GCN Circ. 24705; Insight-HXMT/HE detection: Yi et al., GCN Circ. 24713; Konus-Wind observation: Svinkin et al., GCN Circ. 24730) triggered the CALET Gamma- ray Burst Monitor (CGBM) at 20:10:20.034 UTC on 31 May 2019. The burst signal was seen by all CGBM detectors. No real-time CGBM GCN notice was distributed about this trigger because the real-time communication from the ISS was off (loss of signal). The burst light curve shows a multi- peaked emission episode which starts at T-9.7 sec, peaks at 14.5 sec and ends at T+74.5 sec. The T90 and T50 durations measured by the SGM data are 36.8 +- 20.0 sec and 13.5 +- 0.9 sec (40-1000 keV), respectively. The ground processed light curve is available at http://cgbm.calet.jp/cgbm_trigger/ground/1243368627/ The CALET data used in this analysis are provided by the Waseda CALET Operation Center located at the Waseda University. |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/287633]  |
| 专题 | 硬X射线调制望远镜卫星 |
| 作者单位 | 中国科学院高能物理研究所 |
| 推荐引用方式 GB/T 7714 | Shimizu, Y,Yoshida, A,Sakamoto, T,et al. GRB 190531B: CALET Gamma-Ray Burst Monitor detection. 2019. |
入库方式： OAI收割
来源：高能物理研究所
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