{
  "bibcode": "2019GCN.26433....1X",
  "body": "S. Xiao, Y. G. Zheng, C. Cai, Q. Luo, Q. B. Yi, \nY. Huang, C. K. Li, G. Li, X. B. 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\nInsight-HXMT was taking data normally around the reported LIGO/Virgo \nS191213g event (GCN #26402), trigger time 2019-12-13T04:34:08 UTC. \nAt T0, about 79% of the LIGO localization region was covered by the \nInsight-HXMT without occultationby the Earth.\n\nWithin T0 +/- 100 s, no significant excess events (SNR > 3 sigma) are \nfound in a search of the Insight-HXMT/HE raw light curves.\n\nAssuming the GW counterpart GRB with three typical GRB Band spectral \nmodels, two typical duration timescales (1 s, 10 s) from the center \nof the LIGO-Virgo location probability map (RA=331.44 deg, DEC=-42.11 deg), \nthe 5-sigma upper-limits fluence (0.2 - 5 MeV, incident energy) are \nreported below:\n\nBand model 1 (alpha=-1.9, beta=-3.7, Ep=70 keV):\n1 s:   2.8e-07 erg cm^-2\n10 s:  9.0e-06 erg cm^-2\n\nBand model 2 (alpha=-1.0, beta=-2.3, Ep=230 keV):\n1 s:   3.2e-07 erg cm^-2\n10 s:  1.1e-06 erg cm^-2\n\nBand model 3 (alpha=-0.0, beta=-1.5, Ep=1000 keV):\n1 s:   3.3e-07 erg cm^-2\n10 s:  1.4e-06 erg cm^-2\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 spacecraft.",
  "circularId": 26433,
  "createdOn": 1576409216000,
  "email": "xiaoshuo@ihep.ac.cn",
  "subject": "LIGO/Virgo S191213g: Upper limits from Insight-HXMT/HE observations",
  "submitter": "Shuo Xiao at IHEP  <xiaoshuo@ihep.ac.cn>",
  "eventId": "LIGO/Virgo S191213g"
}