{
  "bibcode": "2013GCN.15332....1F",
  "body": "G. Fitzpatrick (UCD) and S. Xiong (UAH) report on behalf of the Fermi GBM\nTeam:\n\nAt 05:09:00.20 UT on 14 October 2013, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 131014A (trigger 403420143/131014215).\nHigh peak flux from the GRB caused GBM to issue a repoint request\nthat reoriented the satellite to place the GRB near the LAT boresight\nfor 2.5 hours, subject to Earth limb contraints.\n\nThe on-ground calculated location, using the GBM trigger\ndata, is RA = 101.9 , DEC = -20.0  (J2000 degrees,\nequivalent to 06h 47m, -20d 0.0'), with an uncertainty\nof 1.00  degrees (radius, 1-sigma containment,\nstatistical only; there is additionally a systematic\nerror which is currently estimated to be 2 to 3 degrees).\nThe angle from the Fermi LAT boresight is 71.9  degrees.\n\nThe GBM light curve consists of a single peak\nwith a duration (T90) of about 3.2 s (50-300 keV).\nThe event fluence (10-1000 keV) in this time interval is\n1.9E-4 +/- 2E-7 erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0+1.3 s in the 10-1000 keV band is 311.5 +/- 1.3 ph/s/cm^2.\n\nThe time-averaged spectrum from T0-1.0 s to T0+4.2 s is\nadequately fit by a Band function with Epeak = 318 +/- 3 keV,\nalpha = -0.34 +/- 0.01, and beta = -2.58 +/- 0.02\n\nThe spectral analysis results presented above are preliminary;\nfinal results will be published in the GBM GRB Catalog.",
  "circularId": 15332,
  "createdOn": 1381756437000,
  "email": "gerard.fitzpatrick@ucdconnect.ie",
  "subject": "GRB 131014A: Fermi GBM detection",
  "submitter": "Gerard Fitzpatrick at UCD  <gerard.fitzpatrick@ucdconnect.ie>",
  "eventId": "GRB 131014A"
}