{
  "bibcode": "2016GCN.19932....1V",
  "body": "P Veres (UAH), A von Kienlin (MPE) and C Meegan (UAH)\nreport on behalf of the Fermi GBM Team:\n\n\"At 11:30:19.286 UT on 17 September 2016, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 160917A (trigger 495804623 / 160917479).\nwhich was also detected by the Swift/BAT\n��� ���\n(Racusin et al., GCN 19926).\n��� ���\nThe GBM on-ground location is consistent with the Swift position.\n\n\nThe angle from the Fermi LAT boresight at the GBM trigger time is 46\ndegrees.\n\n\nThe GBM light curve consists of a single peak\nwith a duration (T90) of about 47 s (50-300 keV).\nThe time-averaged spectrum from T0 to T0+14.1 s is\nbest fit by a power law function with an exponential\nhigh-energy cutoff.  The power law index is -1.00 +/- 0.05 and\nthe cutoff energy, parameterized as Epeak, is 1604 +/- 357 keV.\n\n\nThe event fluence (10-1000 keV) in this time interval is\n(7.2 +/- 0.3)E-6 erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0 in the 10-1000 keV band\nis 5.1 +/- 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": 19932,
  "createdOn": 1474158834000,
  "email": "veresp@gmail.com",
  "subject": "GRB 160917A: Fermi GBM observation",
  "submitter": "Peter Veres at UAH  <veresp@gmail.com>",
  "eventId": "GRB 160917A"
}