{
  "bibcode": "2014GCN.15717....1C",
  "body": "J. R. Cummings reports on behalf of the Swift-BAT team:\n\nThere were some small gaps in the data used in the BAT refined analysis\nof GRB 140108A (Cummings et. al, GCN circ # 15710).  With a complete\ndata set, T90 is slightly shorter, 94 +- 4 seconds, the photon index for\nthe simple power-law fit to the spectrum is slightly larger, 1.62 +- 0.05,\nand the total fluence is slightly larger, (7.0 +- 0.2) x 10^-7 ergs/cm^2.\nThe energy interval is 15-150 keV and uncertainties are 90% confidence.\n\nIn the lightcurve, the second peak is a little larger than it looked\nbefore, and is very similar to the first peak.\n\nThe updated results have been posted at:\nhttp://gcn.gsfc.nasa.gov/notices_s/583338/BA/",
  "circularId": 15717,
  "createdOn": 1389371303000,
  "email": "james.r.cummings@nasa.gov",
  "subject": "GRB 140108A BAT refined analysis update",
  "submitter": "Jay R. Cummings at NASA/GSFC/Swift  <james.r.cummings@nasa.gov>",
  "eventId": "GRB 140108A"
}