{
  "bibcode": "2019GCN.26081....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 2019-10-25T18:42:09.10 (T0), Insight-HXMT/HE detected \nGRB 191025A (trigger ID: HEB191025779) in a routine search of the data, \nwhich was also triggered by INTEGRAL/SPIACS (Trigger Number: 8394) and \nKonus-Wind. \n\nThe Insight-HXMT/HE light curve mainly consists of multiple \npulses with a duration (T90) of 0.145 s measured from T0+0.03 s. \nThe 1-ms peak rate, measured from T0+0.123 s, is 63021 cnts/sec. \nThe total counts from this burst is 2544 counts. The data of \nInsight-HXMT/HE suffers saturation in the brightest part.\nURL_LC: http://www.hxmt.org/images/GRB/HEB191025779_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": 26081,
  "createdOn": 1572233483000,
  "email": "luoqi@ihep.ac.cn",
  "subject": "GRB 191025B: Insight-HXMT/HE detection",
  "submitter": "Qi Luo at IHEP  <luoqi@ihep.ac.cn>",
  "eventId": "GRB 191025B"
}