{
  "bibcode": "2010GCN.10852....1S",
  "body": "T. Sakamoto (GSFC/UMBC), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC),\nJ. R. Cummings (GSFC/UMBC), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA),\nC. B. Markwardt (GSFC/UMD), D. M. Palmer (LANL), M. Stamatikos (GSFC/ORAU),\nG. Stratta (ASDC), J. Tueller (GSFC), T. N. Ukwatta (GWU)\n(i.e. the Swift-BAT team):\n \nUsing the data set from T-239 to T+963 sec from recent telemetry downlinks,\nwe report further analysis of BAT GRB 100614A (trigger #424716)\n(Stratta, et al., GCN Circ. 10837).  The BAT ground-calculated position is\nRA, Dec = 263.534, 49.232 deg which is \n   RA(J2000)  =  17h 34m 08.2s \n   Dec(J2000) = +49d 13' 56.4\" \nwith an uncertainty of 1.6 arcmin, (radius, sys+stat, 90% containment).\nThe partial coding was 56%.\n \nThe mask-weighted light curve shows a relatively smooth peak starting\nat ~T-10 sec, peaking around T+50 sec, and ending at ~T+275 sec.\nT90 (15-350 keV) is 225 +- 55 sec (estimated error including systematics).\n \nThe time-averaged spectrum from T-9.0 to T+282.0 sec is best fit by a simple\npower-law model.  The power law index of the time-averaged spectrum is\n1.88 +- 0.15.  The fluence in the 15-150 keV band is 2.7 +- 0.2 x 10^-6 erg/cm2.\nThe 1-sec peak photon flux measured from T+31.00 sec in the 15-150 keV band\nis 0.7 +- 0.2 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/424716/BA/",
  "circularId": 10852,
  "createdOn": 1276610350000,
  "email": "scott@lheamail.gsfc.nasa.gov",
  "subject": "GRB 100614A: Swift-BAT refined analysis",
  "submitter": "Scott Barthelmy at NASA/GSFC  <scott@lheamail.gsfc.nasa.gov>",
  "eventId": "GRB 100614A"
}