TITLE: GCN CIRCULAR NUMBER: 6571 SUBJECT: GRB 070621: Swift-BAT refined analysis DATE: 07/06/22 13:52:28 GMT FROM: Scott Barthelmy at NASA/GSFC E. Fenimore (LANL), L. Barbier (GSFC), S. D. Barthelmy (GSFC), J. Cummings (GSFC/UMBC), N. Gehrels (GSFC), H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), D. Palmer (LANL), A. Parsons (GSFC), T. Sakamoto (GSFC/ORAU), G. Sato (GSFC/ISAS), B. Sbarufatti (INAF-IASFPA), M. Stamatikos (GSFC/ORAU), J. Tueller (GSFC), T. Ukwatta (GWU) (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 070621 (trigger #282808) (Sbarufatti, et al., GCN Circ. 6560). The BAT ground-calculated position is RA, Dec = 323.806, -24.809 deg which is RA(J2000) = 21h 35m 13.5s Dec(J2000) = -24d 48' 32" with an uncertainty of 1.0 arcmin, (radius, sys+stat, 90% containment). The partial coding was 31%. The mask-weighted light curve shows several overlapping peaks starting at ~T-20 sec and ending at ~T+40 sec. There is a low-significance bump (~3 sigma) from T+70 to T+105 sec. T90 (15-350 keV) is 33.3 +- 1.0 sec (estimated error including systematics). The time-averaged spectrum from T-5.2 to T+36.4 sec is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.57 +- 0.06. The fluence in the 15-150 keV band is 4.3 +- 0.1 x 10^-6 erg/cm2. The 1-sec peak photon flux measured from T+21.56 sec in the 15-150 keV band is 2.5 +- 0.3 ph/cm2/sec. All the quoted errors are at the 90% confidence level.