{
  "bibcode": "2015GCN.18015....1J",
  "body": "P. Jenke (UAH) reports on behalf of the Fermi GBM Team:\n\n\"At 18:23:00.16 UT on July 11 2015, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 150711A (trigger 458331784/150711766),\nwhich was also detected by \nSwift (M. G. Bernardini (INAF-OAB) et al. 2015, GCN 18011). \nThe GBM on-ground location, using the Fermi GBM trigger\ndata, is consistent with the Swift/XRT location.  \n\nThe angle of the burst direction to the Fermi LAT boresight\n is 28 degrees.\n\nThe GBM light curve is a single peak with a \nduration (T90) of about 14s (50-300 keV).\nThe time-averaged spectrum from T0-13s to T0+19s \nis well fit by a power law with an exponential high-energy cutoff. \nThe power law index is -1.16 +/- 0.07\nand the cutoff energy, parameterized as Epeak, is 117 +/- 10 keV. \n\nThe event fluence (10-1000 keV) in this time interval is\n(2.8 +/- 0.06)E-06 ergs/cm^2. The 1.0-sec peak photon flux measured\nstarting from T0+4.7s in the 10-1000 keV band\nis 4.1 +/- 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": 18015,
  "createdOn": 1436666916000,
  "email": "peter.a.jenke@nasa.gov",
  "subject": "GRB 150711A: Fermi GBM detection",
  "submitter": "Peter Jenke at MSFC  <peter.a.jenke@nasa.gov>",
  "eventId": "GRB 150711A"
}