{
  "bibcode": "2015GCN.17295....1S",
  "body": "Matthew Stanbro (UAH) report on behalf of the Fermi GBM Team:\n\n\"At 22:08:31.91 UT on 10 January 2015, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 150110B (trigger 442620514 / 150110923)\nwhich was also detected by the Swift/BAT (Evans et al. 2015, GCN 17291)\nThe GBM on-ground location is consistent with the Swift position.\n\nThe angle from the Fermi LAT boresight is 22 degrees.\n\nThe GBM light curve consists of 1 peak\nwith a duration (T90) of about 2 s (50-300 keV).\nThe time-averaged spectrum from T0-1.54 s to T0+1.54 s is\nbest fit by a power law function with an exponential\nhigh-energy cutoff.  The power law index is -0.98 +/- 0.22 and\nthe cutoff energy, parameterized as Epeak, is 122.5 +/- 24.3 keV\n\nThe event fluence (10-1000 keV) in this time interval is\n(5.30 +/- 0.61)E-07 erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0-0.06 s in the 8-1000 keV band\nis 2.33 +/- 0.21 ph/s/cm^2.\n\nThe spectral analysis results presented above are preliminary;\nfinal results will be published in the GBM GRB Catalog.\"",
  "circularId": 17295,
  "createdOn": 1420956206000,
  "email": "mcs0001@uah.edu",
  "subject": "GRB 150110B: Fermi GBM Detection",
  "submitter": "Matthew Stanbro at UAH/Fermi  <mcs0001@uah.edu>",
  "eventId": "GRB 150110B"
}