{
  "bibcode": "2018GCN.23039....1H",
  "body": "Y. Huang, G. Li, S. L. Xiong, X. B. Li, C. K. Li, C.Z. Liu, \r\nX.F. Li, Z. W. Li, Z. Chang, J. L. Zhao, A. M. Zhang, \r\nY. F. Zhang, X. F. Lu, C. L. Zou (IHEP), Y. J. Jin, \r\nZ. Zhang (THU), T. P. Li (IHEP/THU),F. J. Lu, L. M. Song, \r\nH. Y. Wang, M. Wu, Y. P. Xu, S. N. Zhang (IHEP),\r\nreport on behalf of the Insight-HXMT team:\r\n \r\nAt 2018-07-22T23:49:13.000 (T0), the Insight-HXMT/HE detected\r\nGRB 180722B(trigger ID: HEB180722992) in a routine search of the data,\r\nwhich was also triggered by Fermi-GBM (trigger #553996158), \r\nKonus-Wind (trigger time 23:49:18.90 UT) and CALET \r\n(T. Tamura et al., GCN23028).\r\n \r\nThe Insight-HXMT/HE light curve consists of two broad pulses\r\nwith a duration (T90) of 49.2 s measured from T0+0.4 s.\r\nThe 1-s peak rate, measured from T0+41.5 s, is 1679.3 cnts/sec.\r\nThe total counts from this burst is 27707.0 counts.\r\n \r\nURL_LC: http://www.hxmt.org/images/GRB/HEB180722992_lc.jpg\r\n \r\nAll measurements above are made with the CsI detectors operating in the\r\nregular mode with the energy range of about 80-800 keV (record energy).\r\nOnly gamma-rays with energy greater than about 200 keV can penetrate\r\nthe spacecraft and leave signals in the CsI detectors installed inside\r\nof the telescope.\r\n \r\nThe analysis results presented above are preliminary, \r\nfinal results will be published elsewhere.\r\n  \r\nInsight-HXMT is the first Chinese space X-ray telescope, which was funded\r\njointly by the China National Space Administration (CNSA) and the Chinese\r\nAcademy of Sciences (CAS). More information about it could be found at:\r\nhttp://www.hxmt.org.",
  "circularId": 23039,
  "createdOn": 1532576320000,
  "email": "huangyue@ihep.ac.cn",
  "subject": "GRB 180722B: Insight-HXMT/HE detection",
  "submitter": "Yue Huang at IHEP  <huangyue@ihep.ac.cn>",
  "eventId": "GRB 180722B"
}