{
  "bibcode": "2012GCN.13472....1B",
  "body": "W. H. Baumgartner (GSFC/UMBC), S. D. Barthelmy (GSFC), J. R. Cummings (GSFC/UMBC),\nE. E. Fenimore (LANL), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA),\nC. B. Markwardt (GSFC), D. M. Palmer (LANL), T. Sakamoto (GSFC/UMBC),\nG. Sato (ISAS), C. J. Saxton (UCL-MSSL), M. Stamatikos (OSU),\nJ. Tueller (GSFC), T. N. Ukwatta (MSU)\n(i.e. the Swift-BAT team):\n \nUsing the data set from T-60 to T+243 sec from recent telemetry downlinks,\nwe report further analysis of BAT GRB 120714A (trigger #526593)\n(Saxton, et al., GCN Circ. 13464).  The BAT ground-calculated position is\nRA, Dec = 167.975, -30.625 deg, which is \n   RA(J2000)  =  11h 11m 54.1s \n   Dec(J2000) = -30d 37' 29.8\" \nwith an uncertainty of 1.6 arcmin, (radius, sys+stat, 90% containment).\nThe partial coding was 40%.\n \nThe mask-weighted light curve shows a single FRED-like pulse starting at\n~T-1 sec, peaking at ~T+4 sec, and ending at ~T90 sec.\nT90 (15-350 keV) is 16.2 +- 4.0 sec (estimated error including systematics).\n \nThe time-averaged spectrum from T-0.74 to T+17.78 sec is best fit by a simple\npower-law model.  The power law index of the time-averaged spectrum is\n1.62 +- 0.16.  The fluence in the 15-150 keV band is 8.2 +- 0.9 x 10^-7 erg/cm2.\nThe 1-sec peak photon flux measured from T+3.58 sec in the 15-150 keV band\nis 1.5 +- 0.3 ph/cm2/sec.  All the quoted errors are at the 90% confidence\nlevel. \n \nThe results of the batgrbproduct analysis are available at\nhttp://gcn.gsfc.nasa.gov/notices_s/526593/BA/",
  "circularId": 13472,
  "createdOn": 1342302979000,
  "email": "scott@lheamail.gsfc.nasa.gov",
  "subject": "GRB 120714A: Swift-BAT refined analysis",
  "submitter": "Scott Barthelmy at NASA/GSFC  <scott@lheamail.gsfc.nasa.gov>",
  "eventId": "GRB 120714A"
}