IHEP OpenIR  > 硬X射线调制望远镜卫星
GRB 190531B: CALET Gamma-Ray Burst Monitor detection
Shimizu, Y; Yoshida, A; Sakamoto, T; Pal'Shin, V; Sugita, S; Kawakubo, Y; Yamaoka, K; Nakahira, S; Asaoka, Y; Ozawa, S; Torii, S; Tamura, T; Cannady, N; Cherry, M. L; Ricciarini, S; Marrocchesi, P. S.; Collaboration, Calet
GCN Number24738
2019-06-04
Source PublicationGRB Coordinates Network
AbstractThe 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.
ADS URLhttps://ui.adsabs.harvard.edu/abs/2019GCN.24738....1S
ADS Bibcode2019GCN.24738....1S
GCN URLhttps://gcn.gsfc.nasa.gov/gcn/gcn3/24738.gcn3
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Cited Times:0 [ADS]
Document TypeGCN
Identifierhttp://ir.ihep.ac.cn/handle/311005/287633
Collection硬X射线调制望远镜卫星
Affiliation中国科学院高能物理研究所
Recommended Citation
GB/T 7714
Shimizu, Y,Yoshida, A,Sakamoto, T,et al. GRB 190531B: CALET Gamma-Ray Burst Monitor detection. 2019.
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