{
  "bibcode": "2011GCN.12179....1V",
  "body": "A. von Kienlin (MPE) and Chryssa Kouveliotou (NASA/MSFC) report on behalf of\nthe Fermi GBM Team: \n \n\"At 12:47:54.38 UT on 14 July 2001, the Fermi Gamma-Ray Burst Monitor\ntriggered (trigger 332340476 / 110714533) \non a very short event with a soft spectrum. The source of the emission was\nlater identified as a new source, \nSwift J1822.3-1606 (Cummings et al. GCN Circ. 12159).\n \nThe GBM on-ground location is consistent with the Swift position.\n \nThe event duration is approximately 8 ms. Its spectrum is adequately fit\nwith either an optically thin thermal \nbremsstrahlung (OTTB) model of kT = 37 +/- 5 keV or a power law with an\nexponential cutoff (COMPT) with \nindex = 0.2 +/- 0.6 and Epeak = 40 +/-3 keV. The event fluence (10-1000 keV)\nis ~4 x E-08 erg/cm2. \n \nVisual observation of the GBM data revealed at least three and possibly four\nadditional \nevents near the trigger time ranging in duration between 10 - 30 ms.\nPreliminary analysis indicates a harder \nspectrum for these non-triggered events. \"",
  "circularId": 12179,
  "createdOn": 1311091128000,
  "email": "azk@mpe.mpg.de",
  "subject": "Swift J1822.3-1606 : Fermi GBM observation",
  "submitter": "Andreas von Kienlin at MPE  <azk@mpe.mpg.de>"
}