TITLE: GCN CIRCULAR NUMBER: 7979 SUBJECT: GRB 080714: Swift-BAT refined analysis DATE: 08/07/15 02:59:58 GMT FROM: Jay R. Cummings at NASA/GSFC/Swift S. D. Barthelmy (GSFC), W. Baumgartner (GSFC/UMBC), J. Cummings (GSFC/UMBC), E. Fenimore (LANL), N. Gehrels (GSFC), H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), K. McLean (GSFC/UMD), D. Palmer (LANL), A. Parsons (GSFC), M. Perri (ASDC), T. Sakamoto (GSFC/UMBC), G. Sato (ISAS), M. Stamatikos (GSFC/ORAU), J. Tueller (GSFC), T. Ukwatta (GWU) on behalf of the Swift-BAT team: Using the data set from T-240 to T+963 sec from the recent telemetry downlink, we report further analysis of BAT GRB 080714 (trigger #316910) (Perri, et al., GCN Circ. 7978). The BAT ground-calculated position is RA, Dec = 188.104, -60.274 deg which is RA(J2000) = 12h 32m 24.9s Dec(J2000) = -60d 16' 28.2" with an uncertainty of 1.0 arcmin, (radius, sys+stat, 90% containment). The partial coding was 43%. The mask-weighted lightcurve shows a single peak with a rise time of about 3 seconds and an exponential decay with a time constant of about 10 seconds. T90 (15-350 keV) is 33 +- 9 sec (estimated error including systematics). There is a small peak in the raw light curve, mostly above 25 keV, at about T-90 sec that appears to be from a different source, out of the field of view. The time-averaged spectrum from T-3.6 to T+50.3 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.52 +- 0.08. The fluence in the 15-150 keV band is 2.5 +- 0.1 x 10^-06 erg/cm2. The 1-sec peak photon flux measured from T-0.37 sec in the 15-150 keV band is 4.2 +- 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/316910/BA/