TITLE: GCN CIRCULAR NUMBER: 14219 SUBJECT: GRB 130215A: Fermi GBM detection DATE: 13/02/15 21:10:57 GMT FROM: George A. Younes at USRA/NASA/MSFC George Younes (USRA) and P. N. Bhat (UAH) report on behalf of the Fermi GBM Team: "At 01:31:26.02 UT on 15 February 2013, the Fermi Gamma-Ray Burst Monitor triggered and located GRB 130215A (trigger 382584689 / 130215063). which was also detected by the Swift/BAT (D'Elia et al. 2013, GCN 14204) The GBM on-ground location is consistent with the Swift position. The angle from the Fermi LAT boresight is 86 degrees. The GBM light curve consists of single FRED like pulse with a duration (T90) of about 140 s (50-300 keV). The time-averaged spectrum from T0-7.0 s to T0+124 s is adequately fit by a Band function with Epeak= 155 +/- 63 keV, alpha = -1.0 +/- 0.2 and beta = -1.60 +/- 0.03. The event fluence (10-1000 keV) in this time interval is (2.02 +/- 0.05)E-05 erg/cm^2. The 1-sec peak photon flux measured starting from T0+10.56 s in the 10-1000 keV band is 3.5 +/- 0.3 ph/s/cm^2. The spectral analysis results presented above are preliminary; final results will be published in the GBM GRB Catalog."