GCN Circular 5091
L. Barbier (GSFC), S. Barthelmy (GSFC), J. Cummings (GSFC/ORAU), H. Krimm (GSFC/USRA), C. Markwardt (GSFC/UMD), D. Palmer (LANL), T. Sakamoto (GSFC/ORAU), J. Tueller (GSFC) on behalf of the Swift-BAT team: Now having recieved the full downlinked data that fills in the gaps (Tueller et al, GCN 5090), we report the updated refined analysis on Swift-BAT GRB 060507 (trigger 208870). The lightcurve description in GCN 5090 does not change, nor does T90. The time-averaged spectrum from T-10.2 to T+192.4 is best fit by a simple power-law model. The power law index of the time-averaged spectrum is 1.83 +- 0.09. The fluence in the 15-150 keV band is 4.5 +- 0.2 x 10^-6 erg/cm2. The 1-sec peak photon flux measured from T+1.24 sec in the 15-150 keV band is 1.3 +- 0.2 ph/cm2/sec. All the quoted errors are at the 90% confidence level.