TITLE: GCN CIRCULAR NUMBER: 32737 SUBJECT: Fermi Gamma-ray Burst Monitor continues to detect SGR 1935+2154 DATE: 22/10/13 15:03:24 GMT FROM: Christian Malacaria at ISSI C. Malacaria (ISSI), P. Veres (UAH) and O. Roberts (USRA) report on behalf of the Fermi-GBM Team: "The Fermi Gamma-ray Burst Monitor (GBM) triggers 221013391/687345829 at 09:23:44.18 UT, 221013376/687344475 at 09:01:10.88 UT, 221013334/687340841 at 08:00:36.49 UT, 221013304/687338292 at 07:18:07.15 UT, 221013295/687337536 at 07:05:31.76 UT, 221013037/687315163 at 00:52:38.25 UT on 13 October 2022 and 221012977/687310007 at 23:26:42.31 UT, 221012906/687303863 at 21:44:18.47 UT, 221012874/687301134 at 20:58:49.99 UT, 221012773/687292428 at 18:33:43.51 UT, 221012709/687286852 at 17:00:47.29 UT, on 12 October 2022 all tentatively classified as a GRB, are in fact not due to a GRB. These triggers are due to a SGR 1935+2154 which, as recently announced (Mereghetti et al., GCN #32706 and Roberts et al. GCN #32708), is undergoing high bursting activity. For Fermi GBM data and info, please visit the official Fermi GBM Support Page: https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/"