TITLE: GCN CIRCULAR NUMBER: 16103 SUBJECT: GRB 140412A: Swift-BAT refined analysis DATE: 14/04/13 14:22:16 GMT FROM: Scott Barthelmy at NASA/GSFC T. N. Ukwatta (MSU), S. D. Barthelmy (GSFC), W. H. Baumgartner (GSFC/UMBC), J. R. Cummings (GSFC/UMBC), V. D'Elia (ASDC), N. Gehrels (GSFC), H. A. Krimm (GSFC/USRA), A. Y. Lien (NASA/UMBC), C. B. Markwardt (GSFC), D. M. Palmer (LANL), T. Sakamoto (AGU), M. Stamatikos (OSU), J. Tueller (GSFC) (i.e. the Swift-BAT team): Using the data set from T-240 to T+962 sec from recent telemetry downlinks, we report further analysis of BAT GRB 140412A (trigger #595608) (D'Elia, et al., GCN Circ. 16097). The BAT ground-calculated position is RA, Dec = 145.032, -65.826 deg, which is RA(J2000) = 09h 40m 07.6s Dec(J2000) = -65d 49' 33.7" with an uncertainty of 1.7 arcmin, (radius, sys+stat, 90% containment). The partial coding was 77%. The mask-weighted light curve shows two peaks strting at ~T-35 sec, peaking at ~T+1 sec, and ending at ~T+35 sec. T90 (15-350 keV) is 39.6 +- 8.2 sec (estimated error including systematics). The time-averaged spectrum from T-36.94 to T+12.18 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.95 +- 0.19. The fluence in the 15-150 keV band is 7.2 +- 0.8 x 10^-7 erg/cm2. The 1-sec peak photon flux measured from T+0.04 sec in the 15-150 keV band is 1.1 +- 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/595608/BA/