{
  "bibcode": "2005GCN..4104....1B",
  "body": "L. Barbier (GSFC), S. Barthelmy (GSFC), J. Cummings (GSFC/NRC),\nE. Fenimore (LANL), N. Gehrels (GSFC), D. Hullinger (GSFC/UMD),\nH. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), F. Marshall (GSFC),\nD. Palmer (LANL), A. Parsons (GSFC), T. Sakamoto (GSFC/NRC),\nG. Sato (ISAS), T. Takahashi (ISAS), J. Tueller (GSFC)\non behalf of the Swift-BAT team:\n\nUsing the full data set from the recent telemetry downlink, we report\nfurther analysis of Swift-BAT GRB 051016B (trigger #159994)\n(Parsons, et al., GCN 4103).  The ground-analysis position is\nRA,Dec 132.120,+13.627 {08h 48m 28.8s,+13d 37' 38.4\"} (J2000)\nwith an uncertainty of 1.6 arcmin (radius, 90%, stat+sys).\nThe parital coding fraction is 79 %.  T90 is 4.0 +- 0.1 sec.\nThe lightcurve consists of two overlapping peaks at T+0.3 and T+3.0 sec.\nFitting a simple power law over the full interval from T-0.0 to T+4.6 sec,\nthe photon index is 2.38 +/- 0.23 with a fluence of 1.7 +/- 0.2 X 10^-7\nerg/cm^2.  The peak flux in a 1-sec wide window starting at T+0.11 sec\nis 1.32 +/- 0.17 ph/cm^2/sec.  All values are in the 15-150 keV band\nat the 90% confidence level.",
  "circularId": 4104,
  "createdOn": 1129501902000,
  "email": "Scott@lheamail.gsfc.nasa.gov",
  "subject": "GRB 051016B:  Refined analysis of the Swift-BAT burst",
  "submitter": "Scott Barthelmy at NASA/GSFC  <Scott@lheamail.gsfc.nasa.gov>",
  "eventId": "GRB 051016B"
}