{
  "bibcode": "2016GCN.20049....1B",
  "body": "S. D. Barthelmy (GSFC), J. R. Cummings (GSFC/UMBC), N. Gehrels (GSFC),\nH. A. Krimm (GSFC/USRA), A. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC),\nD. M. Palmer (LANL), J. L. Racusin (NASA/GSFC), T. Sakamoto (AGU),\nM. Stamatikos (OSU), T. N. Ukwatta (LANL)\n(i.e. the Swift-BAT team):\n\nUsing the data set from T-240 to T+962 sec from the recent telemetry downlink,\nwe report further analysis of BAT GRB 161014A (trigger #717500)\n(Racusin, et al., GCN Circ. 20035).  The BAT ground-calculated position is\nRA, Dec = 332.626, 7.467 deg which is\n    RA(J2000)  =  22h 10m 30.1s\n    Dec(J2000) = +07d 28' 01.9\"\nwith an uncertainty of 1.5 arcmin, (radius, sys+stat, 90% containment).\nThe partial coding was 13%.\n\nThe mask-weighted light curve shows a complex structure starting at T-10 sec\nand ending at T+15 sec.  T90 (15-350 keV) is 18.3 +- 2.8 sec (estimated error\nincluding systematics).\n\nThe time-averaged spectrum from T-9.1 to T+12.5 sec is best fit by a simple\npower-law model.  The power law index of the time-averaged spectrum is\n1.47 +- 0.15.  The fluence in the 15-150 keV band is 1.9 +- 0.2 x 10^-6 erg/cm2.\nThe 1-sec peak photon flux measured from T+0.10 sec in the 15-150 keV band\nis 2.9 +- 0.6 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/717500/BA/",
  "circularId": 20049,
  "createdOn": 1476540249000,
  "email": "tsakamoto@phys.aoyama.ac.jp",
  "subject": "GRB 161014A: Swift-BAT refined analysis",
  "submitter": "Takanori Sakamoto at AGU  <tsakamoto@phys.aoyama.ac.jp>",
  "eventId": "GRB 161014A"
}