[vsnet-grb-info 6496] GLAST Burst Monitor detection of GRB080816
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Tue Aug 19 21:09:58 JST 2008
TITLE: GCN CIRCULAR
NUMBER: 8107
SUBJECT: GLAST Burst Monitor detection of GRB080816
DATE: 08/08/19 12:09:51 GMT
FROM: Andreas von Kienlin at MPE <azk at mpe.mpg.de>
Andreas von Kienlin, Sheila McBreen and Elisabetta Bissaldi (MPE)
report on behalf of the GLAST Burst Monitor Team:
"At 12:04:18 UT on 2008 Aug 16, the GLAST Burst Monitor (GBM)
triggered and located GRB 080816 (GBM 080816.503 / trigger 240581059).
The on-ground calculated location, using the GBM trigger data, is
RA = 156.9, Dec = +54.60 (J2000 degrees)
(equivalent to J2000 10h 28m, +54d 36'),
with an uncertainty of 2.3 degrees (radius, 1-sigma containment, statistical
only; there is additionally a systematic error which is currently estimated
to be 2 to 3 degrees). The angle from the Large Area Telescope (LAT)
boresight is 55 degrees at ~T+35 sec.
This GRB has a duration of approximately 70 s and contains 4 peaks.
The preliminary averaged time spectrum in the 10 keV to 500 keV energy band
from T-1 to T+69 s is well fit by a power law function with an exponential
high energy cutoff. The power law index is -0.57 +/-0.14 and the cutoff
energy, parameterized as Epeak, is 146.7 +/-14.5 keV, with a reduced
chi-square of 1.2 for 291 degrees of freedom.
The fluence in the 50-300 keV band is (1.86 +/- 0.20) x 10^-5 erg/cm2.
The 1-sec photon flux measured from T+35 sec in the 50-300 keV band
is 3.48 +/-0.66 ph/cm2/sec. All the quoted errors are at the 90%
confidence level.
These spectral analysis results presented above are preliminary; the final
results will be published in the GBM GRB Catalog."
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