TITLE: GCN GRB OBSERVATION REPORT NUMBER: 5334 SUBJECT: GRB 060714: Refined analysis of the Swift-BAT burst DATE: 06/07/17 20:35:56 GMT FROM: Scott Barthelmy at NASA/GSFC H. Krimm (GSFC/USRA), L. Barbier (GSFC), S. D. Barthelmy (GSFC), J. Cummings (GSFC/ORAU), E. Fenimore (LANL), N. Gehrels (GSFC), D. Hullinger (BYU-Idaho), M. Koss (GSFC/UMD), C. Markwardt (GSFC/UMD), D. Palmer (LANL), A. Parsons (GSFC), T. Sakamoto (GSFC/ORAU), G. Sato (GSFC/ISAS), M. Stamatikos (GSFC/ORAU), J. Tueller (GSFC) on behalf of the Swift-BAT team: Using the data set from T-240 to T+962 sec from the telemetry downlinks, we report further analysis of BAT GRB 060714 (trigger #219101) (Krimm, et al., GCN Circ. 5311). The BAT ground-calculated position is RA,Dec = 227.854, -6.545 deg {15h 11m 24.9s, -6d 32' 42.3"} (J2000) +- 1.5 arcmin, (radius, sys+stat, 90% containment). The partial coding was 27%. The mask-weighted lightcurves show an initial triangular-shapped peak starting at T-15 sec, peaking at T_zero, and ending at T+55. Then come two peaks, each about 20 sec FWHM, peaking at T+76 and T+90 sec; the last peak ending at T+120 sec. We note that the XRT follow-up observation does not start until the trailing edge of the second peak. T90 (15-350 keV) is 115 +- 5 sec (estimated error including systematics). The time-averaged spectrum from T-13.3 to T+120.6 is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.99 +- 0.10. The fluence in the 15-150 keV band is 3.0 +- 0.2 x 10^-6 erg/cm2. The 1-sec peak photon flux measured from T+75.42 sec in the 15-150 keV band is 1.4 +- 0.1 ph/cm2/sec. All the quoted errors are at the 90% confidence level. We apologize for the long delay in issuing this standard BAT Second Circular.