[vsnet-grb-info 7821] GRB 090515: Swift-BAT refined spectral analysis
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Sat May 16 00:29:26 JST 2009
TITLE: GCN CIRCULAR
NUMBER: 9365
SUBJECT: GRB 090515: Swift-BAT refined spectral analysis
DATE: 09/05/15 15:29:10 GMT
FROM: Takanori Sakamoto at NASA/GSFC <takanori.sakamoto-1 at nasa.gov>
T. Sakamoto (GSFC/UMBC), A. P. Beardmore (U Leicester)
on behalf of the Swift-BAT team
Based on a further analysis of the BAT spectrum of GRB 090515
(Barthelmy, et al. , GCN Circ. 9364), we found that the spectrum shows
a significant improvement of chi2 by a power-law with an exponential
cutoff (chi squared 52.55 for 56 d.o.f.) over a simple power-law
(chi squared 58.63 for 57 d.o.f.). This fit gives a photon index
-0.05 +- 1.36, and Epeak of 64 +- 23 keV. For this model
the total fluence in the 15-150 keV band is 2.0 +- 0.3 x 10^-8 erg/cm2.
All the quoted errors are at the 90% confidence level.
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