{
  "bibcode": "2013GCN.14189....1G",
  "body": "A. Goldstein (UAH) reports on behalf of the Fermi GBM Team:\n\nAt 19:36:30.45 UT on 06 February 2013, the Fermi Gamma-Ray \nBurst Monitor triggered and located GRB 130206A \n(trigger 381872193 /130206817) which was also detected by \nthe Swift/BAT (De Pasquale et al. 2013, GCN 14181).  The GBM \non-ground location is consistent with the Swift position.\nThe angle from the Fermi LAT boresight is 19 degrees.\n\nThe GBM light curve consists of three overlapping pulses \nwith a duration (T90) of about 91 s (50-300 keV). The \ntime-averaged spectrum from T0=-1.5 s to T0+85.6 s is \nadequately fit by a power law function with an exponential \nhigh-energy cutoff.  The power law index is -1.1 +/- 0.2 and \nthe cutoff energy, parameterized as Epeak, is 132.6 +/- 34.0 keV.\n\nThe event fluence (10-1000 keV) in this time interval is \n(3.3 +/- 0.4)E-6 erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0+1.8 s in the 10-1000 keV band is \n2.1 +/- 0.2 ph/s/cm^2.\n\nThe spectral analysis results presented above are preliminary;\nfinal results will be published in the GBM GRB Catalog.",
  "circularId": 14189,
  "createdOn": 1360275698000,
  "email": "adam.m.goldstein@msfc.nasa.gov",
  "subject": "GRB 130206A: Fermi GBM observation",
  "submitter": "Adam Goldstein at Fermi-GBM/UAH  <adam.m.goldstein@msfc.nasa.gov>",
  "eventId": "GRB 130206A"
}