IHEP OpenIR  > 硬X射线调制望远镜卫星
GRB 190610A: CALET Gamma-Ray Burst Monitor detection
Tamura, T; Yoshida, A; Sakamoto, T; Pal'Shin, V; Sugita, S; Kawakubo, Y; Yamaoka, K; Nakahira, S; Asaoka, Y; Ozawa, S; Torii, S; Shimizu, Y; Cannady, N; Cherry, M. L; Ricciarini, S; Marrocchesi, P. S.; Collaboration, Calet
GCN Number24805
Source PublicationGRB Coordinates Network
AbstractThe short GRB 190610A (Swift-BAT trigger #907754: Evans et al., GCN Circ. 24775, Palmer et al., GCN Circ. 24783; Insight-HXMT/HE detection: Cai et al., GCN Circ. 24782) triggered the CALET Gamma-ray Burst Monitor (CGBM) at 11:27:45.359 UTC on 10 June 2019. The burst signal was seen by all CGBM detectors. The burst light curve shows a single pulse which starts at T+0.58 sec, peaks at T+0.83 sec and ends at T+1.41 sec. The T90 and T50 durations measured by the SGM data are 0.61 +- 0.16 sec and 0.26 +- 0.05 sec (40-1000 keV), respectively. The ground processed light curve is available at http://cgbm.calet.jp/cgbm_trigger/ground/1244201256/ 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.24805....1T
ADS Bibcode2019GCN.24805....1T
GCN URLhttps://gcn.gsfc.nasa.gov/gcn/gcn3/24805.gcn3
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Cited Times:0 [ADS]
Document TypeGCN
Recommended Citation
GB/T 7714
Tamura, T,Yoshida, A,Sakamoto, T,et al. GRB 190610A: CALET Gamma-Ray Burst Monitor detection. 2019.
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