{
  "bibcode": "2019GCN.25879....1L",
  "body": "Q. Luo, C. Cai, S. Xiao, Q. B. Yi, Y. G. Zheng, Y. Huang, \nC. K. Li, X. B. Li, G. Li, J. Y. Liao, S. L. Xiong, \nC. Z. Liu, X. F. Li, Z. W. Li, Z. Chang, A. M. Zhang, \nY. F. Zhang, X. F. Lu, C. L. Zou (IHEP), Y. J. Jin, \nZ. Zhang (THU), T. P. Li (IHEP/THU), F. J. Lu, L. M. Song, \nM. Wu, Y. P. Xu, S. N. Zhang (IHEP), \nreport on behalf of the Insight-HXMT team:\n\nAt 2019-09-28T13:12:14.00 (T0), Insight-HXMT/HE detected \nGRB 190928A (trigger ID: HEB190928550) in a routine search of the data, \nwhich was also reported by AGILE/MCAL (GCN #25859), IPN triangulation \n(GCN #25864), CALET/GBM (GCN #25865) and Konus-Wind (GCN #25868). \n\nThe Insight-HXMT/HE light curve mainly consists of multiple \npulses with a duration (T90) of 31.10 s measured from T0+78.39 s. \nThe 1-ms peak rate, measured from T0+102.88 s, is 23712 cnts/sec. \nThe total counts from this burst is 152469 counts. The data of \nInsight-HXMT/HE suffers saturation in the brightest part.\nURL_LC: http://www.hxmt.org/images/GRB/HEB190928550_lc.jpg \n\nAll measurements above are made with the CsI detectors operating in the \nregular mode with the energy range of about 80-800 keV (deposited energy). \nOnly gamma-rays with energy greater than about 200 keV can penetrate \nthe spacecraft and leave signals in the CsI detectors installed inside \nof the telescope. \n\nInsight-HXMT is the first Chinese space X-ray telescope, which was \nfunded jointly by the China National Space Administration (CNSA) and \nthe Chinese Academy of Sciences (CAS). \nMore information about it could be found at: \nhttp://www.hxmt.org.",
  "circularId": 25879,
  "createdOn": 1569858641000,
  "email": "luoqi@ihep.ac.cn",
  "subject": "GRB 190928A: Insight-HXMT/HE detection",
  "submitter": "Qi Luo at IHEP  <luoqi@ihep.ac.cn>",
  "eventId": "GRB 190928A"
}