{
  "submittedHow": "web",
  "eventId": "GRB 251214D",
  "createdOn": 1765806423888,
  "submitter": "Xinghao Luo at SVOM/GRM <2952704891@qq.com>",
  "bibcode": "2025GCN.43121....1L",
  "format": "text/plain",
  "subject": "GRB 251214D: GECAM-B observation of a long burst",
  "body": "Xing-Hao Luo, Chen-Wei Wang, Shao-Lin Xiong (IHEP) report on behalf of GECAM team:\n\nGECAM-B was triggered on-ground by GRB 251214D, at 2025-12-14T21:24:17.950 UTC (denoted as T0), which is also detected by AstroSat/CZTI (A. Arya et.al., GCN #43109).\n\nAccording to the GECAM-B light curves in about 70-6000 keV, this burst mainly consists of multiple pulses with a duration (T90) of  28.5 +6.5/-5.0 s.\n\nThe GECAM-B light curve can be found here:\nhttps://www.bursthub.cn//admin/static/gecambgrb251214D.png\n\nGravitational wave high-energy Electromagnetic Counterpart All-sky Monitor (GECAM) mission originally consists of two micro-satellites (GECAM-A and GECAM-B) launched in Dec. 2020. As the third member of GECAM constellation, GECAM-C was launched onboard SATech-01 experimental satellite in July 2022. GECAM mission is funded by the Chinese Academy of Sciences (CAS).\n",
  "circularId": 43121
}