{
  "bibcode": "2005GCN..4063....1P",
  "body": "D. Palmer (LANL), L. Barbier (GSFC), S. Barthelmy (GSFC),\nJ. Cummings (GSFC/NRC), E. Fenimore (LANL), N. Gehrels (GSFC),\nK. Gendreau (GSFC), D. Hullinger (GSFC/UMD), H. Krimm (GSFC/USRA),\nC. Markwardt (GSFC/UMD), P. Meszaros (PSU), A. Parsons (GSFC),\nT. Sakamoto (GSFC/NRC), G. Sato (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 Trigger #158593 (Norris, et al., GCN 4061).\nThe ground-analysis position is RA,Dec 110.808,+9.510\n{7h 23m 13.8s,+9d 30' 36.3\"} (J2000) with an uncertainty\nof 1.7 arcmin (radius, 90%, stat+sys).  T90 is 26 +- 1 sec.\nThe lightcurve has an initial cluster of 3 overlapping peaks at T-5 to T+8 sec\nand a fourth peak at T+20 sec.  Fitting a simple power law\nover the full interval from T-5.9 to T+24.7 sec, the photon index\nis 1.4 +/- 0.2 with a fluence of 1.28 +/- 0.13 X 10^-6 erg/cm^2.\nThe peak flux in a 1-sec wide window starting at T+3.2 sec\nis 1.9 +/- 0.3 ph/cm^2/sec.  All values are in the 15-150 keV band\nat the 90% confidence level.",
  "circularId": 4063,
  "createdOn": 1128640549000,
  "email": "Scott@lheamail.gsfc.nasa.gov",
  "subject": "GRB051006: Refined analysis of the Swift-BAT burst",
  "submitter": "Scott Barthelmy at NASA/GSFC  <Scott@lheamail.gsfc.nasa.gov>",
  "eventId": "GRB 051006"
}