{
  "subject": "GRB 231110A: GECAM-B detection (correction)",
  "createdOn": 1699756007785,
  "bibcode": "2023GCN.34992....1W",
  "eventId": "GRB 231110A",
  "circularId": 34992,
  "body": "Yue Wang, Shao-Lin Xiong, Yue Huang report on behalf of the GECAM team:\n\nGECAM-B was triggered in-flight by a long burst, GRB 231110A, at 2023-11-10T21:19:35.100 UTC (T0), which was also observed by Swift/BAT (GCN #34977).\n\nAccording to the realtime alert data of GECAM-B, this burst\nmainly consists of a long pulse with a duration (T90) of about ~20 sec (20-1000 keV).\n\nThe GECAM-B localization is consistent with the Swift/BAT localization (trigger=1195733) within the error.\n\nThe time-averaged spectrum of GECAM-B realtime data from about T0 to T0+4 s could be\nadequately fit by a cut-off power-law with a flux about 1.3E-6 erg/cm^2/s in 20-1000 keV. \n\nWe note that these results are based on realtime alert data and thus very preliminary. \nRefined analysis will be reported later.\n\nGravitational wave high-energy Electromagnetic Counterpart All-sky Monitor\n(GECAM) mission originally consists of two microsatellites (GECAM-A and GECAM-B)\nlaunched in Dec. 2020. As the third member of GECAM constellation, \nGECAM-C was launched onboard SATech-01 experimental satellite in July 2022. \nGECAM mission is funded by the Chinese Academy of Sciences (CAS).",
  "submitter": "Yue Wang <m18509381757@163.com>",
  "submittedHow": "web"
}