{
  "bibcode": "2011GCN.12320....1B",
  "body": "S. D. Barthelmy (GSFC) and T. Sakamoto (GSFC/UMBC),\n(on behalf of the Swift-BAT team):\n\nDue to an error in the automated processing, an incorrect best-fit model\nwas selected in Circ 12317.  The correct best fit model is the simple\nblackbody model.  We apologise for this error.\n\nThe time-averaged spectrum from T+0.000 to T+0.012 sec of the event from\nSGR Swift J1834.9-0846 (BAT Trigger 501752) is best fit by a blackbody model.\nThe blackbody temperature is 9.2 -1.6,+1.4 keV.  The fluence in the 15-150 keV\nband is 5.6 +- 2.6 x 10^-9 erg/cm2.  The 1-sec peak photon flux measured\nfrom T-0.49 sec in the 15-150 keV band is 0.31 +- 0.19 ph/cm2/sec.\nAll the quoted errors are at the 90% confidence level.  \n\nWe thank A.Kann for bringing this fitting choice error to our attention.",
  "circularId": 12320,
  "createdOn": 1314900178000,
  "email": "scott@lheamail.gsfc.nasa.gov",
  "subject": "SGR Swift J1834.9-0846: Correction to the Swift-BAT refined spectral analysis",
  "submitter": "Scott Barthelmy at NASA/GSFC  <scott@lheamail.gsfc.nasa.gov>"
}