{
  "bibcode": "2014GCN.16066....1P",
  "body": "V. Pelassa (UAH), G. Fitzpatrick (UCD), C. Meegan and N. Bhat (UAH)\nreport on behalf of the Fermi GBM Team:\n\n\"At 04:19:54.47 UT on 30 March 2014, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 140330A (trigger 417845997 / 140330180),\nwhich was also detected by Konus-Wind (S. Golenetskii et al, GCN 16056)\nand localized by the Interplanetary Network (K. Hurley et al, GCN 16051).\nThe GBM on-ground location is consistent with the IPN location.\nThe angle from the Fermi LAT boresight is 13.6 degrees.\n\nThe GBM light curve consists of a FRED pulse with a duration (T90)\nof about 34 s (50-300 keV).\n\nThe time-averaged spectrum from T0-0.768 s to T0+35.073 s is\nwell fit by a power law function with an exponential\nhigh-energy cutoff. The power law index is -0.66 +/- 0.10 and\nthe cutoff energy, parameterized as Epeak, is 197 +/- 17 keV.\n(Castor statistics 578.62 for 486 d.o.f.).\nA Band function fits the spectrum equally well (Castor statistics\n577.22 for 485 d.o.f.) with Epeak= 172 +/- 23 keV,\nalpha = -0.57 +/- 0.13 and beta = -2.4 +/- 0.3.\nThis result is consistent with the analysis of the Konus observation\n(S. Golenetskii et al, GCN 16056).\n\nThe event fluence (10-1000 keV) in this time interval is\n(5.6 +/- 0.3)E-06  erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0+0.640 s in the 10-1000 keV band\nis 4.3 +/- 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": 16066,
  "createdOn": 1396322684000,
  "email": "vero.pelassa@gmail.com",
  "subject": "GRB 140330A: Fermi GBM observation",
  "submitter": "Veronique Pelassa at UAH  <vero.pelassa@gmail.com>",
  "eventId": "GRB 140330A"
}