TITLE: GCN CIRCULAR NUMBER: 14916 SUBJECT: GRB 130612A: Swift-BAT refined analysis DATE: 13/06/19 22:01:54 GMT FROM: Craig Markwardt at NASA/GSFC C. B. Markwardt (GSFC), S. D. Barthelmy (GSFC), T. Sakamoto (AGU), on behalf of the Swift-BAT team: Using the data set from T-25 to T+100 sec from the recent telemetry downlink, we report further analysis of BAT GRB 130612A (trigger #557976) (Racusin, et al., GCN Circ. 14874). The BAT ground-calculated position is RA, Dec = 259.771, 16.729 deg which is RA(J2000) = 17h 19m 05.0s Dec(J2000) = +16d 43' 44.7" with an uncertainty of 2.0 arcmin, (radius, sys+stat, 90% containment). The partial coding was 34%. The mask weighted light curve shows a single FRED-like profile with a rise time of about 1 sec near T+0sec and a gradual decay time with e-folding time of about 3 sec. This burst was detected as the Swift spacecraft was entering the South Atlantic Anomaly region, and the raw background counting rate was ramping upward. The mask weighted light curve does not have a clean background level, so estimating the T90 is difficult. If we restrict the analysis to the time range T-25 to T+100, we estimate T90 (15-350 keV) to be 4.0 +/- 1.4 sec. However, we cannot rule out the possibility of a faint extended emission tail to approximately T+100 (in which case T90 is 110 +/- 60 sec). The time-averaged spectrum from T-0.83 to T+3.17 sec is best fit by a power law with an exponential cutoff. This fit gives a photon index -0.14 +- 1.71, and Epeak of 36.4 +- 7.6 keV (chi squared 36 for 56 d.o.f.). For this model the total fluence in the 15-150 keV band is 2.3 +- 0.5 x 10^-7 erg/cm2 and the 1-sec peak flux measured from T+0.17 sec in the 15-150 keV band is 1.7 +- 0.3 ph/cm2/sec. A fit to a simple power law gives a photon index of 2.06 +- 0.25 (chi squared 44 for 57 d.o.f.). 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/557976/BA/