TITLE: GCN CIRCULAR NUMBER: 19705 SUBJECT: GRB 160714A: Swift-BAT refined analysis, DATE: 16/07/14 14:10:23 GMT FROM: Takanori Sakamoto at AGU D. M. Palmer (LANL), S. D. Barthelmy (GSFC), J. R. Cummings (GSFC/UMBC), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), A. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC), D. M. Palmer (LANL), T. Sakamoto (AGU), M. H. Siegel (PSU), M. Stamatikos (OSU), T. N. Ukwatta (LANL) (i.e. the Swift-BAT team): Using the data set from T-239 to T+963 sec from the recent telemetry downlink, we report further analysis of BAT GRB 160714A (trigger #704310) (Siegel, et al., GCN Circ. 19697). The BAT ground-calculated position is RA, Dec = 234.490, 63.809 deg which is RA(J2000) = 15h 37m 57.7s Dec(J2000) = +63d 48' 32.1" with an uncertainty of 2.7 arcmin, (radius, sys+stat, 90% containment). The partial coding was 35%. The mask-weighted light curve shows a double-peak structure starting at T0, peaking at T+0.05 sec and T+0.2 sec and ending at T+0.3 sec. T90 (15-350 keV) is 0.35 +- 0.11 sec (estimated error including systematics). The time-averaged spectrum from T+0.02 to T+0.40 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.38 +- 0.37. The fluence in the 15-150 keV band is 6.9 +- 1.6 x 10^-8 erg/cm2. The 1-sec peak photon flux measured from T-0.29 sec in the 15-150 keV band is 1.1 +- 0.3 ph/cm2/sec. All the quoted errors are at the 90% confidence level. The results of the batgrbproduct analysis are available at http://gcn.gsfc.nasa.gov/notices_s/704310/BA/