{
  "bibcode": "2022GCN.32737....1M",
  "body": "C. Malacaria (ISSI), P. Veres (UAH) and O. Roberts (USRA) \nreport on behalf of the Fermi-GBM Team:\n\n\"The Fermi Gamma-ray Burst Monitor (GBM) triggers \n221013391/687345829 at 09:23:44.18 UT,\n221013376/687344475 at 09:01:10.88 UT, \n221013334/687340841 at 08:00:36.49 UT, \n221013304/687338292 at 07:18:07.15 UT,\n221013295/687337536 at 07:05:31.76 UT, \n221013037/687315163 at 00:52:38.25 UT\non 13 October 2022 and\n221012977/687310007 at 23:26:42.31 UT,\n221012906/687303863 at 21:44:18.47 UT,\n221012874/687301134 at 20:58:49.99 UT,\n221012773/687292428 at 18:33:43.51 UT,\n221012709/687286852 at 17:00:47.29 UT,\non 12 October 2022\nall tentatively classified as a GRB, are in fact not due to a GRB.\n\nThese triggers are due to a SGR 1935+2154 which, \nas recently announced (Mereghetti et al., GCN #32706 and \nRoberts et al. GCN #32708), is undergoing high bursting activity.\n\nFor Fermi GBM data and info, please visit\nthe official Fermi GBM Support Page:\nhttps://fermi.gsfc.nasa.gov/ssc/data/access/gbm/\"",
  "circularId": 32737,
  "createdOn": 1665673404000,
  "email": "cmalacaria.astro@gmail.com",
  "subject": "Fermi Gamma-ray Burst Monitor continues to detect SGR 1935+2154",
  "submitter": "Christian Malacaria at ISSI  <cmalacaria.astro@gmail.com>",
  "eventId": "SGR 1935+2154"
}