TITLE: GCN CIRCULAR NUMBER: 34249 SUBJECT: GRB 230723B: Fermi GBM observation DATE: 23/07/24 14:00:22 GMT FROM: Joe Mangan at IJCLab J.Mangan (CNRS/IJCLab) and C. Meegan (UAH) report on behalf of the Fermi GBM Team: At 11:42:33.03 UT on 23 July 2023, the Fermi Gamma-Ray Burst Monitor (GBM) triggered and located GRB 230723B (trigger 711805358 / 230723488), which was also detected by Swift BAT (K. L. Page et al. 2023, GCN 34234). The Fermi GBM on-ground location is consistent with the Swift BAT position. The angle from the Fermi LAT boresight at the GBM trigger time is 78 degrees. The GBM light curve consists of a single peak with a duration (T90) of about 10 s (50-300 keV). The time-averaged spectrum from T0-2 s to T0+9 s is best fit by a power law function with an exponential high-energy cutoff. The power law index is -0.9 +/- 0.1 and the cutoff energy, parameterized as Epeak, is 59.1 +/- 2.7 keV. The event fluence (10-1000 keV) in this time interval is (3.8 +/- 0.2)E-06 erg/cm^2. The 1-sec peak photon flux measured starting from T0+1.2 s in the 10-1000 keV band is 7.8 +/- 0.4 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/