TITLE: GCN CIRCULAR NUMBER: 21416 SUBJECT: GRB 170804A: Swift-BAT refined analysis DATE: 17/08/05 15:45:14 GMT FROM: Amy Lien at GSFC H. A. Krimm (NSF/USRA), S. D. Barthelmy (GSFC), A. Cholden-Brown (PSU), J. R. Cummings (CPI), A. Y. Lien (GSFC/UMBC), C. B. Markwardt (GSFC), D. M. Palmer (LANL), T. Sakamoto (AGU), M. Stamatikos (OSU), T. N. Ukwatta (LANL) (i.e. the Swift-BAT team): Using the data set from T-240 to T+962 sec from the recent telemetry downlink, we report further analysis of BAT GRB 170804A (trigger #766194) (Cholden-Brown et al., GCN Circ. 21410). The BAT ground-calculated position is RA, Dec = 6.404, -64.781 deg which is RA(J2000) = 00h 25m 37.0s Dec(J2000) = -64d 46' 50.9" with an uncertainty of 1.3 arcmin, (radius, sys+stat, 90% containment). The partial coding was 75%. The mask-weighted light curve shows several over-lapping pulses that start at ~T0 and end at ~T+60 s. T90 (15-350 keV) is 43.4 +- 9.8 sec (estimated error including systematics). The time-averaged spectrum from T+1.98 to T+60.90 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.67 +- 0.13. The fluence in the 15-150 keV band is 1.3 +- 0.1 x 10^-6 erg/cm2. The 1-sec peak photon flux measured from T+25.10 sec in the 15-150 keV band is 0.9 +- 0.2 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/766194/BA/