TITLE: GCN CIRCULAR NUMBER: 35763 SUBJECT: GRB 240215B: Fermi GBM Observation DATE: 24/02/20 16:45:45 GMT FROM: Lorenzo Scotton at UAH <lscottongcn@outlook.com> L. Scotton (UAH) and C. Meegan (UAH) report on behalf of the Fermi Gamma-ray Burst Monitor Team: "At 19:51:43.85 UT on 15 February 2024, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 240215B (trigger 729719508/240215828), which was also detected by Swift/BAT-GUANO (J. DeLaunay et al. 2024, GCN 35739), and GRBAlpha (A. Pal et al. 2024, GCN 35752). The Fermi GBM Final Real-time Localization was reported in GCN 35740, but was mislabelled as GRB 240215C. After manual inspection, a more accurate on-ground location was found to be RA = 309.52, Dec = -48.74, with a statistical uncertainty of 2.54 degrees. The angle from the Fermi LAT boresight is 94 degrees. The GBM light curve consists of a single emission episode with a duration (T90) of about 21 s (50-300 keV). The time-averaged spectrum from T0-5.5 to T0+21.5 s is best fit by a power law function with an exponential high-energy cutoff. The power law index is -1.16 +/- 0.04 and the cutoff energy, parameterized as Epeak, is 210 +/- 10 keV. The event fluence (10-1000 keV) in this time interval is (1.12 +/- 0.04)E-05 erg/cm^2. The 1-sec peak photon flux measured starting from T0+4.9 s in the 10-1000 keV band is 10.8 +/- 0.4 ph/s/cm^2. A Band function fits the spectrum equally well with Epeak= 190 +/- 20 keV, alpha = -1.13 +/- 0.05 and beta = -2.5 +/- 0.3. The spectral analysis results presented above are preliminary; final results will be published in the GBM GRB Catalog: https://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html For Fermi GBM data and info, please visit the official Fermi GBM Support Page: https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/" View this GCN Circular online at https://gcn.nasa.gov/circulars/35763. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...