{
  "bibcode": "2005GCN..4194....1B",
  "body": "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),\nT. Mitani (ISAS), D. Palmer (LANL), A. Parsons (GSFC), T. Sakamoto (GSFC/NRC), \nG. Sato (ISAS), M. Suzuki (Saitama), J. Tueller (GSFC), \non behalf of the Swift/BAT team:\n\nWe have re-analyzed GRB 051105 (GCN Circ 4188, Mineo et al., and \nGCN Circ 4190, Cummings et al.) based on new time interval T0\nto T0 + 0.120 sec.\n\nThe improved refined BAT ground position is (RA,Dec) = 265.277, 34.949, \n{17h 41m  6.6s, 34d 56' 56.8\"} [deg; J2000] +- 2.5 arcmin, \n(90% containment). The partial coding was 81%.  \n\nThe photon index of the time-averaged spectrum is 1.33 +- 0.35 \nin the time interval TO + 0.122 sec. The fluence in the 15-150 keV \nband is (2.0 +- 0.46) x 10^-8 erg/cm2. The peak photon flux in the \nsame time window measured in the 15-150 band is (2.0 +- 0.43) \nph/cm2/sec.  All the quoted errors are at the 90% confidence level.",
  "circularId": 4194,
  "createdOn": 1131207739000,
  "email": "lmb@cosmicra.gsfc.nasa.gov",
  "subject": "GRB 051105: Swift-BAT improved refined analysis",
  "submitter": "Louis M Barbier at NASA/GSFC/Swift  <lmb@cosmicra.gsfc.nasa.gov>",
  "eventId": "GRB 051105"
}