{
  "bibcode": "2011GCN.12073....1X",
  "body": "Shaolin Xiong (UAH)\nreports on behalf of the Fermi GBM Team:\n\n\"At 15:21:32.549 UT on 10 June 2011, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 110610A (trigger 329412094 / 110610640),\nwhich was also detected by the Swift/BAT (Marshall et al. 2011, GCN 12065).\nThe GBM on-ground location is consistent with the Swift position.\nThis burst was also detected by INTEGRAL SPI-ACS and Suzaku WAM.\n\nThe angle from the Fermi LAT boresight is 59 degrees.\n\nThe GBM light curve consists of multiple peaks\nwith a duration (T90) of about 40 s (50-300 keV).\nThe time-averaged spectrum from T0+0.0 s to T0+39.4 s is\nbest fit by a power law function with an exponential\nhigh-energy cutoff. The power law index is -0.97 +/- 0.05 and\nthe cutoff energy, parameterized as Epeak, is 189.9 +/- 14.0 keV.\nThe event fluence (10-1000 keV) in this time interval is\n(8.70 +/- 0.35)E-06 erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0+33.7 s in the 10-1000 keV band is 5.97 +/- 0.25 ph/s/cm^2.\n\nA Band function fits the spectrum equally well with\nEpeak = 170.0 +/- 19.8 keV, alpha = -0.93 +/- 0.07\nand beta = -2.23 +/- 0.20.\n\nThe spectral analysis results presented above are preliminary;\nfinal results will be published in the GBM GRB Catalog.\"",
  "circularId": 12073,
  "createdOn": 1308098544000,
  "email": "sx0002@uah.edu",
  "subject": "GRB 110610A: Fermi GBM detection",
  "submitter": "Shaolin Xiong at UAH  <sx0002@uah.edu>",
  "eventId": "GRB 110610A"
}