TITLE: GCN CIRCULAR NUMBER: 29374 SUBJECT: Fermi GBM Observations of SGR J1935+2154 DATE: 21/01/29 23:56:51 GMT FROM: Oliver J Roberts at USRA/NASA O.J. Roberts (USRA), J. Wood (USRA), A. von Kienlin (MPE), P. Veres (UAH) and G. Younes (GWU) report on behalf of the Fermi GBM Team: "At 15:23:29.92 UT on January 29th 2020, the Fermi Gamma-Ray Burst Monitor (GBM) triggered and located a burst from SGR 1935+2154 (trigger 633626614 / 210129641). SGR J1935 bursts have also been reported by Konus-Wind (Ridnaia et al., GCN 29373), GECAM (Y. Huang et al., GCN 29363) and Swift-BAT (Ridania et al., GCN 29365). The GBM on-ground location is consistent with the known position of the SGR. The burst has a duration (T90) of about 0.1 seconds. There are two additional bursts that also appear to be from SGR J1935, about 354s after the trigger time. It is adequately fit by a power law function with an exponential high-energy cutoff. The power law index is 0.2 (+0.2/-0.2) and the cutoff energy, parameterized as Epeak, is 32.9 (+0.6/-0.6) keV. The event fluence (10-1000 keV) from T0-0.064s to T0+0.064s is (5.2 +/- 0.1)E-7 erg/cm^2. The average photon flux in the 10-1000 keV band during this period is 94.6 +/- 1.9 ph/s/cm^2. The spectrum is also well fit using a double blackbody (BB+BB) fit, with low and high temperatures of 6.2 (+0.6/-0.7) and 12.5 (+1.6/-1.3) keV, respectively. Fermi GBM also subsequently triggered on multiple bursts from SGR J1935+2154 on January 24th, 28th and today, with a fraction of these being misclassified as GRBs. These triggers are: January 29th: 210129886 / 633647760 (21:15:55.98 UTC) 210129441 / 633609344 (10:35:39.94 UTC) 210129116 / 633581187 (02:46:22.58 UTC) January 28th 210128983 / 633569707 (23:35:02.48 UTC) January 24th 210124867 / 633214108 (20:48:24.00 UTC) 210124325 / 633167319 (07:48:34.36 UTC) The spectral analysis results presented above are preliminary. For Fermi GBM data and info, please visit the official Fermi GBM Support Page: https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/”