{
  "bibcode": "2005GCN..4033....1C",
  "body": "J. Cummings (GSFC/NRC), L. Barbier (GSFC), S. Barthelmy (GSFC), \nE. Fenimore (LANL), N. Gehrels (GSFC), D. Hullinger (UMD), \nH. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), D. Palmer (LANL), \nA. Parsons (GSFC), T. Sakamoto (GSFC/NRC), G. Sato (ISAS), \nJ. Tueller (GSFC)\non behalf of the Swift-BAT team:\n\nWe report a correction to Hullinger et al. (GCN circ. 4019).  There\nare two additional peaks in the interval T+260 to T+275 sec besides \nthe broader, somewhat more intense peaks reported earlier.  We had \nmistakenly stated that there was no emission after T+120.  We have \nno mask-weighted data from T+300 to T+330 sec, but the raw rates show \nno peaks in this interval.  There is no significant emission after \nT+330 sec; in particular, there does not seem to be any emission in \nthe BAT energy range at the times of the Xray flares reported by Godet \net al. (GCN circ. 4031).\n\nThe two later peaks are softer, shorter, and sharper.  The total\nfluence from T+0 to T+300 sec is (2.6 +- 0.4) x 10^-6 ergs/cm^2 in the \n15-150 keV band.  The power-law photon index for the total burst is \n2.1 +- 0.2.  T90 is 250 +- 20 sec.  Errors are 90% confidence \nincluding systematics.",
  "circularId": 4033,
  "createdOn": 1127602442000,
  "email": "jayc@milkyway.gsfc.nasa.gov",
  "subject": "GRB 050922B: Correction to BAT refined analysis, longer burst",
  "submitter": "Jay R. Cummings at NASA/GSFC/Swift  <jayc@milkyway.gsfc.nasa.gov>",
  "eventId": "GRB 050922B"
}