{
  "bibcode": "2021GCN.31236....1Z",
  "body": "Y. Q. Zhang, S. L. Xiong, X. B. Li, C. Cai, Q. Luo, S. Xiao, \nJ. C. Liu, W. C. Xue, Q. B. Yi, C. Zheng���Y. Huang, C. K. Li, \nG. Li, J. Y. Liao, X. Y. Song, S. L. Xiong, C. Z. Liu, \nX. F. Li, Z. W. Li, Z. Chang, A. M. Zhang, Y. F. Zhang, \nX. F. Lu, C. L. Zou (IHEP), Y. J. Jin, Z. Zhang (THU), \nT. 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 2021-12-11T13:09:59.500 (T0), Insight-HXMT/HE detected \nGRB 211211A (trigger ID: HEB211211548) in a routine search of the data, \nwhich also triggered Fermi/GBM (Fermi GBM Team, GCN #31201),\nSwift/BAT (D'Ai A. et al., GCN #31202),  \nCALET (Tamura T. et al., GCN #31226) and\nINTEGRAL/SPI-ACS (Minaev P. et al., GCN #31230)\n\nURL_LC: http://twiki.ihep.ac.cn/pub/HXMT/GRBList/HEB211211548_lc.jpg\n\nIt should be noted that there is a significant saturation effect (data loss)\nduring bright parts of this GRB in HXMT. \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": 31236,
  "createdOn": 1639637050000,
  "email": "yqzhang@ihep.ac.cn",
  "subject": "GRB 211211A: Insight-HXMT/HE detection",
  "submitter": "Y Q Zhang at IHEP  <yqzhang@ihep.ac.cn>",
  "eventId": "GRB 211211A"
}