{
  "bibcode": "2016GCN.20032....1U",
  "body": "T. N. Ukwatta (LANL), S. D. Barthelmy (GSFC),\nJ. R. Cummings (GSFC/UMBC), V. D'Elia (ASDC),\nN. Gehrels (GSFC), H. A. Krimm (GSFC/USRA),\nA. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC),\nD. M. Palmer (LANL), T. Sakamoto (AGU),\nM. Stamatikos (OSU), (i.e. the Swift-BAT team):\n\nUsing the data set from T-790 to T+963 sec from the recent telemetry downlink,\nwe report further analysis of BAT GRB 161011A (trigger #716876)\n(D'Elia, et al. GCN Circ. 20023).  The BAT ground-calculated position is\nRA, Dec = 245.687, 8.313 deg which is\n   RA(J2000)  =  16h 22m 44.9s\n   Dec(J2000) = +08d 18' 47.3\"\nwith an uncertainty of 2.4 arcmin, (radius, sys+stat, 90% containment).\nThe partial coding was 43%.\n\nThe mask-weighted light curve shows a weak single-pulse structure that\nstarts at ~T0, peaks at ~ T+1 s, and ends at ~T+5 s. T90 (15-350 keV) is\n4.3 +- 1.3 sec (estimated error including systematics).\n\nThe time-averaged spectrum from T-0.3 to T+4.4 sec is best fit by a simple\npower-law model.  The power law index of the time-averaged spectrum is\n1.15 +- 0.35.  The fluence in the 15-150 keV band is 2.3 +- 0.4 x 10^-7 erg/cm2.\nThe 1-sec peak photon flux measured from T+1.37 sec in the 15-150 keV band\nis 0.9 +- 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/716876/BA/",
  "circularId": 20032,
  "createdOn": 1476241736000,
  "email": "amy.y.lien@nasa.gov",
  "subject": "GRB 161011A, Swift-BAT refined analysis",
  "submitter": "Amy Lien at GSFC  <amy.y.lien@nasa.gov>",
  "eventId": "GRB 161011A"
}