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编号24805
2019-06-13
出处GRB Coordinates Network
摘要The 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
引用统计
被引频次:0 [ADS]
文献类型GCN
条目标识符https://ir.ihep.ac.cn/handle/311005/287638
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
Tamura, T,Yoshida, A,Sakamoto, T,et al. GRB 190610A: CALET Gamma-Ray Burst Monitor detection. 2019.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
GCN24805.txt(1KB)GCN 限制开放CC BY-NC-SA请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Tamura, T]的文章
[Yoshida, A]的文章
[Sakamoto, T]的文章
百度学术
百度学术中相似的文章
[Tamura, T]的文章
[Yoshida, A]的文章
[Sakamoto, T]的文章
必应学术
必应学术中相似的文章
[Tamura, T]的文章
[Yoshida, A]的文章
[Sakamoto, T]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。