[vsnet-grb-info 6689] GRB 080920: Fermi GBM detection
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Thu Sep 25 22:55:58 JST 2008
TITLE: GCN CIRCULAR
NUMBER: 8290
SUBJECT: GRB 080920: Fermi GBM detection
DATE: 08/09/25 13:55:36 GMT
FROM: Andreas von Kienlin at MPE <azk at mpe.mpg.de>
A. von Kienlin (MPE), E. Bissaldi (MPE), S. McBreen (MPE)
report on behalf of the Fermi GBM Team:
"At 06:25:48 UT on 20 September 2008, the Fermi Gamma-ray Burst Monitor
triggered and located GRB 080920 (trigger 243584749 / 080920268).
The on-ground calculated location using the Fermi GBM trigger data is
RA = 124.6, Dec = 1.6 (equivalent to J2000 08h 18m, 01d 36'),
with a statistical uncertainty of 3.4 degrees
(radius, 1-sigma containment; there is additionally a systematic
error which is currently estimated to be 2 to 3 degrees).
The angle from the Fermi LAT boresight is 16 degrees.
This long GRB comprises one FRED like pulse, starting at T0-6 s.
T90 (25-1000 keV) is about 85 s. The time-averaged spectrum
from T0-6 to T0+79 s is adequately fit by a power law model
with index -1.42 +/- 0.06. It can also be fit with a power
law function with an exponential high energy cutoff.
The cutoff energy, parameterized as Epeak, is 162 +/- 35 keV.
In this case the power law index is poorly constrained (-0.63 +/- 0.25).
The fluence in the 25-1000 keV band is 2.4 (+/- 0.5) E-06 erg/cm2
and the peak flux (25-1000 keV) on the 1 s timescale
is 1.29 (+/- 0.14) ph/cm2/s.
The spectral analysis results presented above are preliminary;
final results will be published in the Fermi GBM GRB Catalog."
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