GCN Circular 14858
G. Fitzpatrick (UCD) and V. Pelassa (UAH) report on behalf of the Fermi GBM Team: At 03:12:10.50 UT on 10 June 2013, the Fermi Gamma-Ray Burst Monitor triggered and located GRB 130610A (trigger 392526733 /130610133) which was also detected by the Swift/BAT (Cummings et al., GCN Circ. 14842). The GBM on-ground location is consistent with the Swift position. The GBM light curve consists of a single peak with a duration (T90) of about 28 s (50-300 keV). The time-averaged spectrum from T0-2.6 s to T0+25.7 s is adequately fit by a power law function with an exponential high-energy cutoff. The power law index is -1.0 +/- 0.1 and the cutoff energy, parameterized as Epeak, is 294.9 +/- 42.9 keV The event fluence (10-1000 keV) in this time interval is (6.1 +/- 0.4)E-06 erg/cm^2. The 1-sec peak photon flux measured starting from T0+8.0 s in the 10-1000 keV band is 4.5 +/- 0.9 ph/s/cm^2. The spectral analysis results presented above are preliminary; final results will be published in the GBM GRB Catalog.