[vsnet-grb-info 3256] GRB 060507: Final Refined analysis of the
Swift-BAT burst
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Tue May 9 06:19:02 JST 2006
TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 5091
SUBJECT: GRB 060507: Final Refined analysis of the Swift-BAT burst
DATE: 06/05/08 21:18:07 GMT
FROM: Scott Barthelmy at NASA/GSFC <Scott at lheamail.gsfc.nasa.gov>
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.
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