{
  "bibcode": "2014GCN.16539....1M",
  "body": "C. B. Markwardt (GSFC), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), \nJ. R. Cummings (GSFC/UMBC), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA),\nA. Y. Lien (NASA/UMBC), F. E. Marshall (NASA/GSFC), D. M. Palmer (LANL), \nT. Sakamoto (AGU), M. Stamatikos (OSU), J. Tueller (GSFC), T. N. Ukwatta (MSU)\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 140706A (trigger #603587)\n(Marshall, et al., GCN Circ. 16531).  The BAT ground-calculated position is\nRA, Dec = 49.269, -38.058 deg which is \n  RA(J2000)  =  03h 17m 04.6s \n  Dec(J2000) = -38d 03' 28.6\" \nwith an uncertainty of 1.1 arcmin, (radius, sys+stat, 90% containment).\nThe partial coding was 77%.\n\nThe mask-weighted light curve shows several peaks starting at ~T-20 sec, \npeaking at ~T-15, ~T+1 and ~T+28 sec, and ending at ~T+40 sec.  \nT90 (15-350 keV) is 48.3 +- 4.3 sec (estimated error including systematics).\n\nThe time-averaged spectrum from T-21.3 to T+39.6 sec is best fit by a simple\npower-law model.  The power law index of the time-averaged spectrum is\n1.8 +- 0.1.  The fluence in the 15-150 keV band is 2.0 +- 0.1 x 10^-6 erg/cm2.\nThe 1-sec peak photon flux measured from T-0.12 sec in the 15-150 keV band\nis 1.8 +- 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/603587/BA/",
  "circularId": 16539,
  "createdOn": 1404768648000,
  "email": "tsakamoto@phys.aoyama.ac.jp",
  "subject": "GRB 140706A: Swift-BAT refined analysis",
  "submitter": "Takanori Sakamoto at AGU  <tsakamoto@phys.aoyama.ac.jp>",
  "eventId": "GRB 140706A"
}