GCN Circular 28120
C. Malacaria (NASA-MSFC/USRA), E. Bissaldi (Politecnico and INFN Bari), R. Dunwoody (UCD), J. Mangan (UCD) and C. Meegan (UAH) report on behalf of the Fermi GBM Team: "At 01:26:37.76 UT on 16 July 2020, the Fermi Gamma-Ray Burst Monitor (GBM) triggered and located GRB 200716A (trigger 616555602 / 200716060) , which also triggered AGILE (Ursi A. et al., GCN #28116) and AstroSat (Gupta et al., GCN #28117). The Fermi GBM Final Real-time Localization is reported in GCN #28109. The angle from the Fermi LAT boresight at the GBM trigger time is 76 degrees. The GBM light curve shows multiple peaks with a duration (T90) of about 45 s (50-300 keV). The time-averaged spectrum from T0-9.5 s to T0+59.1 s is best fit by a Comptonized model with Epeak = 456 +/- 17 keV and alpha = -0.97 +/- 0.01 . The event fluence (10-1000 keV) in this time interval is (5.986 +/- 0.041)E-05 erg/cm^2. The 1-sec peak photon flux measured starting from T0+31 s in the 10-1000 keV band is 24.0 +/- 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/"