{
  "bibcode": "2014GCN.16893....1K",
  "body": "H. A. Krimm (GSFC/USRA), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC),\nJ. R. Cummings (GSFC/UMBC), V. D'Elia (ASDC), N. Gehrels (GSFC),\nA. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC), D. M. Palmer (LANL),\nT. Sakamoto (AGU), M. Stamatikos (OSU), J. Tueller (GSFC), T. N. Ukwatta (LANL)\n(i.e. the Swift-BAT team):\n \nUsing the data set from T-239 to T+963 sec from the recent telemetry downlink,\nwe report further analysis of BAT GRB 141005A (trigger #614415)\n(D'Elia, et al., GCN Circ. 16882).  The BAT ground-calculated position is\nRA, Dec = 291.103, 36.098 deg, which is \n   RA(J2000)  =  19h 24m 24.7s \n   Dec(J2000) = +36d 05' 54.1\" \nwith an uncertainty of 1.7 arcmin, (radius, sys+stat, 90% containment).\nThe partial coding was 6%.\n \nThe mask-weighted light curve shows a single peak starting at ~T-1 sec,\npeaking at ~T+2 sec, and ending at ~T+7 sec.  T90 (15-350 keV) is 4.34 +- 1.08 sec\n(estimated error including systematics).\n \nThe time-averaged spectrum from T+0.19 to T+5.66 sec is best fit by a simple\npower-law model.  The power law index of the time-averaged spectrum is\n1.33 +- 0.18.  The fluence in the 15-150 keV band is 1.1 +- 0.1 x 10^-6 erg/cm2.\nThe 1-sec peak photon flux measured from T+0.68 sec in the 15-150 keV band\nis 4.2 +- 0.8 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/614415/BA/",
  "circularId": 16893,
  "createdOn": 1412529545000,
  "email": "scott@lheamail.gsfc.nasa.gov",
  "subject": "GRB 141005A: Swift-BAT refined analysis",
  "submitter": "Scott Barthelmy at NASA/GSFC  <scott@lheamail.gsfc.nasa.gov>",
  "eventId": "GRB 141005A"
}