{
  "bibcode": "2016GCN.19916....1H",
  "body": "R. Hamburg (UAH)\nreports on behalf of the Fermi GBM Team:\n\n\"At 16:10:11.39 UT on 12 September 2016, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 160912A (trigger 495389415 / 160912674).\n\nThis burst was also detected by the Swift BAT approximately\n150 s after the Swift trigger time and reported as an x-ray flare\napproximately 89 arcseconds from the BAT onboard position\n(Cannizzo et al. 2016, GCN 19912). At the time of the Swift trigger,\nthe source was occulted by the Earth for Fermi.\nThe GBM on-ground location is consistent with the Swift position.\n\nThe GBM light curve consists of multiple peaks\nwith a duration (T90) of about 48 s (10-1000 keV).\nThe time-averaged spectrum from T0-4 s to T0+42 s is\nbest fit by a simple power law function with index -1.48 +/- 0.03.\n\nThe event fluence (10-1000 keV) in this time interval is\n(6.1 +/- 0.3)E-06 erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0+8.4 s in the 10-1000 keV band\nis 1.6 +/- 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": 19916,
  "createdOn": 1473736980000,
  "email": "rkh0007@uah.edu",
  "subject": "GRB 160912A: Fermi GBM detection",
  "submitter": "Rachel Hamburg at UAH  <rkh0007@uah.edu>",
  "eventId": "GRB 160912A"
}