{
  "bibcode": "2006GCN..5304....1H",
  "body": "D. Hullinger (BYU-Idaho), L. Barbier (GSFC), S. D. Barthelmy (GSFC),\nJ. Cummings (GSFC/ORAU), E. Fenimore (LANL), N. Gehrels (GSFC),\nH. Krimm (GSFC/USRA), M. Koss (GSFC/UMD), C. Markwardt (GSFC/UMD), \nD. Palmer (LANL), A. Parsons (GSFC), T. Sakamoto (GSFC/ORAU),\nG. Sato (GSFC/ISAS), M. Stamatikos (GSFC/ORAU), J. Tueller (GSFC)\non behalf of the Swift-BAT team:\n\nUsing the data set from T-119 to T+183 sec from recent telemetry downlinks,\nwe report further analysis of BAT GRB 060712 (trigger #218582)\n(Cummings, et al., GCN Circ. 5301).  The BAT ground-calculated position\nis RA,Dec = 184.065, +35.539 deg {12h 16m 15.7s, +35d 32' 21.6\"} (J2000)\n+- 2.2 arcmin, (radius, sys+stat, 90% containment).  The partial coding was 9%.\n \nThe lightcurve for this weak source shows approximately 3 overlapping peaks\nstarting at T_zero and lasting unit ~T+35 sec.  T90 (15-350 keV) is 26 +- 5 sec\n(estimated error including systematics).\n \nThe time-averaged spectrum from T+0.6 to T+29.7 is best fit by a simple\npower-law model.  The power law index of the time-averaged spectrum\nis 1.64 +- 0.32.  The fluence in the 15-150 keV band is\n1.3 +- 0.2 x 10^-6 erg/cm2.  The 1-sec peak photon flux measured\nfrom T+16.76 sec in the 15-150 keV band is 1.7 +- 0.6 ph/cm2/sec.\nAll the quoted errors are at the 90% confidence level.",
  "circularId": 5304,
  "createdOn": 1152755227000,
  "email": "scott@lheamail.gsfc.nasa.gov",
  "subject": "GRB 060712:  Refined analysis of the Swift-BAT burst",
  "submitter": "Scott Barthelmy at NASA/GSFC  <scott@lheamail.gsfc.nasa.gov>",
  "eventId": "GRB 060712"
}