{
  "bibcode": "2014GCN.16592....1Y",
  "body": "H.-F. Yu (MPE) reports on behalf of the Fermi GBM Team:\n\n\"At 06:25:55.42 UT on 14 July 2014, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 140714A (trigger 427011958 / 140714268).\n\nThe trigger resulted in an Autonomous Repoint Request (ARR) that was\naccepted and the spacecraft slewed to the GBM in-flight location.\n\nThe on-ground calculated location, using the GBM trigger data, is \nRA = 221.0, Dec = 40.3 (J2000 degrees, equivalent to 14h 44m, 40d 18'), \nwith an uncertainty of 1.1 degrees (radius, 1-sigma containment, \nstatistical only; there is additionally a systematic error which is \ncurrently estimated to be 2 to 3 degrees).\n\nThe initial angle from the Fermi LAT boresight, using the GBM\non-ground calculated location, is 68 degrees.\n\nThe GBM light curve consists of two main emission episodes,\nwith a duration (T90) of about 132 s (50-300 keV).\nThe time-averaged spectrum from T0+100.353 s to T0+129.026 s is\nwell fit by a Band function with Epeak = 81.9 +/- 2.3 keV,\nalpha = -0.84 +/- 0.04, and beta = -2.8 +/- 0.1.\n\nThe event fluence (10-1000 keV) in this time interval is\n(1.57 +/- 0.03)E-05 erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0+113.794 s in the 10-1000 keV band\nis 15.6 +/- 0.4 ph/s/cm^2.\n\nThe spectral analysis results presented above are preliminary;\nfinal results will be published in the GBM GRB Catalog.\"",
  "circularId": 16592,
  "createdOn": 1405439600000,
  "email": "sptfung@mpe.mpg.de",
  "subject": "GRB 140714A: Fermi GBM detection",
  "submitter": "Hoi-Fung Yu at MPE  <sptfung@mpe.mpg.de>",
  "eventId": "GRB 140714A"
}