GRB 200111A: CALET Gamma-Ray Burst Monitor detection
文献类型：GCN
| 作者 | Torii, S; Yoshida, A; Sakamoto, T; Pal'Shin, V; Sugita, S; Kawakubo, Y; Yamaoka, K; Nakahira, S; Asaoka, Y; Shimizu, Y |
| 发表日期 | 2020-01-17 |
| 出处 | GRB Coordinates Network |
| 英文摘要 | The long GRB 200111A (Fermi GBM Final Real-time Localization: The Fermi GBM team, GCN Circ. 26705; Insight-HXMT/HE detection: Xiao et al., GCN Circ. 26714; IPN triangulation: Hurley et al., GCN Circ. 26778; AstroSat CZTI detection: Gaikwad et al., GCN Circ. 26783; https://gcn.gsfc.nasa.gov/other/200111A.gcn3) triggered the CALET Gamma- ray Burst Monitor (CGBM) at 15:11:07.610 UTC on 11 January 2020. The burst signal was seen by all CGBM detectors. The burst light curve shows a multi-peaked structure followed by a short pulse. The emission starts at T+0.0 sec, peaks at T+6.0 sec and ends at T+6.4 sec. The T90 and T50 durations measured by the SGM data are 6.0 +- 0.5 sec and 3.9 +- 1.9 sec (40-1000 keV), respectively. The ground processed light curve is available at http://cgbm.calet.jp/cgbm_trigger/ground/1262790473/ 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/311005/287704]  |
| 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 | Torii, S,Yoshida, A,Sakamoto, T,et al. GRB 200111A: CALET Gamma-Ray Burst Monitor detection. 2020. |
入库方式： OAI收割
来源：高能物理研究所
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