{
  "subject": "GRB 261011A: GECAM-B observation",
  "eventType": [
    "GRB",
    "Gamma-ray Transient"
  ],
  "createdOn": 1791894582322,
  "eventId": "GRB 261011A",
  "submittedHow": "web",
  "body": "Jin-Ye Luo, Chen-Wei Wang, Yue Wang, Shao-Lin Xiong (IHEP) report on behalf of GECAM team: \n\nGECAM-B was triggered on-ground by GRB 261011A at 2026-10-11T13:49:15.250 UTC (denoted as T0), which is also detected by SVOM/ECLAIRs (Huang et al., GCN #45895), Swift/BAT (Cenko et al., GCN #45896; Barthelmy et al., GCN #45930), and Konus-Wind (Ridnaia et al., GCN #45924).\n\nAccording to the GECAM-B light curves in about 70-6000 keV, this burst mainly consists of muplti-pulses with a duration (T90) of 40 +21/-9 s.\n\nThe GECAM-B light curve can be found here:\nhttps://www.bursthub.cn/gcn/2026/gecambgrb261011A.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).",
  "circularId": 45939,
  "submitter": "Jin-Ye Luo <jy_luo2002@163.com>",
  "format": "text/plain"
}