{
  "bibcode": "2005GCN..4275....1S",
  "body": "T. Sakamoto (GSFC/NRC), L. Barbier (GSFC), S. Barthelmy (GSFC),\nJ. Cummings (GSFC/NRC), E. Fenimore (LANL), N. Gehrels (GSFC),\nD. Hullinger (UMD), H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD),\nF. Marshall (GSFC), D. Palmer (LANL), A. Parsons (GSFC),\nG. Sato (ISAS), A. Smale (NASA HQ), J. Tueller (GSFC),\non behalf of the Swift-BAT team:\n\nUsing the full data set from T-4 to T+16 sec (all the data we will\nget on this ground-detected burst), we report further analysis\nof BAT GRB 051114 (trigger #163844) (Cummings, et al., GCN 4272). \nThe BAT ground-calculated position is (RA,Dec) = 226.266d,+60.156d\n{15h 05m 04s,60d 09' 22\"} [deg; J2000] +- 2 arcmin, (radius,\nsys+stat, 90% containment).  The partial coding was 78%. \n\nThe light curve shows two peaks of roughly equal intensity, the \nsecond slightly softer, one from T+0.2 to T+0.9 sec and one from \nT+1.3 to T+2.7 sec.  T90 (15-350 keV) is (2.2 +- 0.3) sec (estimated \nerror including systematics). \n\nThe power law index of the time-averaged spectrum is 1.22 +- 0.27. \nThe fluence in the 15-150 keV band is (1.32 +- 0.24) x 10^-7 erg/cm2. \nThe 1-sec peak photon flux measured from T+0.2 sec in the 15-150 keV\nband is (0.73 +- 0.16) ph/cm2/sec.  All the quoted errors are at the\n90% confidence level.",
  "circularId": 4275,
  "createdOn": 1132095714000,
  "email": "jayc@milkyway.gsfc.nasa.gov",
  "subject": "GRB 051114: Swift-BAT refined analysis",
  "submitter": "Jay R. Cummings at NASA/GSFC/Swift  <jayc@milkyway.gsfc.nasa.gov>",
  "eventId": "GRB 051114"
}