[vsnet-grb-info 9058] GRB 100325A: Fermi GBM detection
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Fri Mar 26 23:27:00 JST 2010
TITLE: GCN CIRCULAR
NUMBER: 10546
SUBJECT: GRB 100325A: Fermi GBM detection
DATE: 10/03/26 14:26:50 GMT
FROM: Andreas von Kienlin at MPE <azk at mpe.mpg.de>
A. von Kienlin (MPE) reports on behalf of the Fermi GBM Team:
"At 06:36:08.02 UT on 25 March 2010, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 100325A (trigger 291191770/100325275).
The on-ground calculated location, using the GBM trigger
data, is RA = 332.3, DEC = -28.6 (J2000 degrees,
equivalent to 22h 09m, -28d 36'), with an uncertainty
of 1.5 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 Fermi LAT boresight is 9 degrees.
The GBM light curve consists of a single structured pulse with a
duration (T90) of 8.3 +/- 1.9 s (8-1000 keV).
The time-averaged spectrum from T0-1.664 s to T0+7.552 s is
best fit by a power law function with an exponential
high energy cutoff. The power law index is -0.45(+0.12/-0.11) and
the cutoff energy, parameterized as Epeak, is 159.3 (+12.7/-10.8) keV
(CSTAT 502 for 482 d.o.f).
The event fluence (8-1000 keV) in this time interval is
(1.99 +/- 0.04)E-06 erg/cm^2. The 1.024-sec peak photon flux measured
starting from T0+0.512 s in the 8-1000 keV band
is 5.0 +/- 0.2 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
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