{
  "bibcode": "2014GCN.16115....1J",
  "body": "P. Jenke (UAH) reports on behalf of the Fermi GBM Team:\n\n\"At 01:26:40.94 UT on April 16 2014, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 140416A (trigger 419304403/140416060).  \nThe GBM on-ground location, using the Fermi GBM trigger\ndata, is RA = 35.4, Dec = 43.9 (J2000 degrees, equivalent to \n02h 21m 36s, 43d 54'), with an uncertainty of 1 \ndegree (radius, 1-sigma containment,\nstatistical only; there is additionally a systematic error which is\ncurrently estimated to be 2 to 3 degrees).\n\nThe angle of the burst direction to the Fermi LAT boresight is \n138 degrees.\n\nThe GBM light curve consists of several peaks with a duration\n (T90) of about 28.5 s (50-300 keV).\nThe time-averaged spectrum from T0-10.0 s to T0+31.0s is\nwell fit by a Band function with Epeak = 78 +/- 2 keV, \nAlpha = -1.01 +/- 0.04 and Beta = -2.44 +/- 0.03.\n\nThe event fluence (10-1000 keV) in this time interval is\n(7.20 +/- 0.06)E-05 erg/cm^2. The 1.0-sec peak photon flux measured\nstarting from T0+6.4 s in the 10-1000 keV band\nis 71 +/- 1 ph/s/cm^2.\n\nThe spectral analysis results presented above are preliminary;\nfinal results will be published in the GBM GRB Catalog.\"",
  "circularId": 16115,
  "createdOn": 1397682528000,
  "email": "peter.a.jenke@nasa.gov",
  "subject": "GRB 140416A: Fermi GBM detection",
  "submitter": "Peter Jenke at MSFC  <peter.a.jenke@nasa.gov>",
  "eventId": "GRB 140416A"
}