TITLE: GCN CIRCULAR NUMBER: 15272 SUBJECT: GRB 130929A, Swift-BAT refined analysis DATE: 13/09/29 17:14:26 GMT FROM: Jay R. Cummings at NASA/GSFC/Swift D. M. Palmer (LANL), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), J. R. Cummings (GSFC/UMBC), E. E. Fenimore (LANL), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), A. Y. Lien (NASA/GSFC/ORAU), C. B. Markwardt (GSFC), F. E. Marshall (NASA/GSFC), T. Sakamoto (AGU), G. Sato (ISAS), M. Stamatikos (OSU), J. Tueller (GSFC), T. N. Ukwatta (MSU) (i.e. the Swift-BAT team): Using the data set from T-70 to T+963 sec from the recent telemetry downlink, we report further analysis of BAT GRB 130929A (trigger #572308) (Marshall, et al., GCN Circ. 15269). The BAT ground-calculated position is RA, Dec = 135.028, -47.554 deg which is RA(J2000) = 09h 00m 06.7s Dec(J2000) = -47d 33' 14.6" with an uncertainty of 1.6 arcmin, (radius, sys+stat, 90% containment). The partial coding was 44%. The mask-weighted light curve shows a single FRED peak. T90 (15-350 keV) is 11.10 +- 2.98 sec (estimated error including systematics). The time-averaged spectrum from T-1.93 to T+11.50 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 2.00 +- 0.18. The fluence in the 15-150 keV band is 6.9 +- 0.8 x 10^-07 erg/cm2. The 1-sec peak photon flux measured from T+1.32 sec in the 15-150 keV band is 1.7 +- 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/572308/BA/