{
  "bibcode": "2014GCN.16762....1J",
  "body": "P. Jenke (UAH) reports on behalf of the Fermi GBM Team:\n\n\"At 19:41:37.57 UT on September 1 2014, the Fermi Gamma-Ray Burst \nMonitor triggered and located \nGRB 140901A (trigger 431293300/140901821). The GBM on-ground \nlocation, using the Fermi GBM trigger data, is consistent with\nthe IPN Triangulation (K. Hurley et al. 2014, GCN 16761).\n\nThe angle of the burst direction to the Fermi LAT boresight is \n97 degrees.\n\nThe GBM light curve consists of a single peak with a duration\n(T90) of about 0.16 s (50-300 keV).\nThe time-averaged spectrum from T0+0.0 s to T0+0.19 s is\nadequately fit by a Band function with Epeak = 1250 +/- 70 keV,\nAlpha =-0.30 +/- 0.04 and Beta = -3.0 +/- 0.1.\n\nThe event fluence (10-1000 keV) in this time interval is\n(4.8 +/- 0.1)E-06 erg/cm^2. The 64 ms peak photon flux measured\nstarting from T0+0.0 s in the 10-1000 keV band\nis 50 +/- 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": 16762,
  "createdOn": 1409684617000,
  "email": "peter.a.jenke@nasa.gov",
  "subject": "GRB 140901A: Fermi GBM detection",
  "submitter": "Peter Jenke at MSFC  <peter.a.jenke@nasa.gov>",
  "eventId": "GRB 140901A"
}