TITLE: GCN CIRCULAR NUMBER: 43835 SUBJECT: GRB 260223A: Fermi GBM Observation DATE: 26/02/25 17:16:57 GMT FROM: Peter Veres at University of Alabama in Huntsville <veresp@gmail.com> P. Veres (UAH) and C. Meegan (UAH) report on behalf of the Fermi Gamma-ray Burst Monitor Team: "At 04:11:09.81 UT on 23 February 2026, the Fermi Gamma-ray Burst Monitor (GBM) triggered and located GRB 260223A (trigger 793512674/260223174), which was also detected by DDOTI (Becerra et al. 2026, GCN 43811), COLIBRI (de Ugarte Postigo et al. 2026, GCNs 43812, 43814 & 43820), SVOM/GRM (Wang et al. 2026, GCN 43815), SVOM/VT (Li et al. 2026, GCN 43816) and Glowbug (Woolf et al. 2026, GCN 43824). The Fermi GBM on-ground location (GCN 43808) is consistent with the DDOTI position. The angle from the Fermi LAT boresight is 33 degrees. The GBM light curve consists of a single emission episode with a duration (T90) of about 39 s (50-300 keV). The time-averaged spectrum from T0-9.2 to T0+51.2 s is best fit by a Band function with Epeak = 70 +/- 6 keV, alpha = -0.76 +/- 0.09, and beta = -1.91 +/- 0.02. The event fluence (10-1000 keV) in this time interval is (2.16 +/- 0.03)E-05 erg/cm^2. The 1-sec peak photon flux measured starting from T0+18 s in the 10-1000 keV band is 10.4 +/- 0.3 ph/s/cm^2. 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/43835. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...