{
  "bibcode": "2013GCN.14903....1X",
  "body": "Shaolin Xiong (UAH) reports on behalf of the Fermi GBM Team:\n\n\"At 23:56:09.74 UT on 14 June 2013, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 130614A (trigger 392946972 / 130614997).\n\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 = 324.18, DEC = -33.89 (J2000 degrees,\nequivalent to 21 h 36 m, -33 d 53 '), with an uncertainty\nof 1.2 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 17 degrees.\n\nThe GBM light curve consists of a 'FRED' shape pulse\nwith a duration (T90) of about 9.3 s (50-300 keV).\nThe time-averaged spectrum from T0 s to T0+9.4 s is\nwell fit by a power law function with an exponential\nhigh-energy cutoff. The power law index is -1.45 +/- 0.04 and\nthe cutoff energy, parameterized as Epeak, is 101 +/- 5 keV.\n\nThe event fluence (10-1000 keV) in this time interval is\n(6.1 +/- 0.2)E-6 erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0+0.19 s in the 10-1000 keV band\nis 20.7 +/- 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": 14903,
  "createdOn": 1371325723000,
  "email": "sx0002@uah.edu",
  "subject": "GRB 130614A: Fermi GBM detection",
  "submitter": "Shaolin Xiong at UAH  <sx0002@uah.edu>",
  "eventId": "GRB 130614A"
}