[vsnet-grb-info 7497] GRB 090328B: Fermi GBM Detection
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Tue Mar 31 03:06:10 JST 2009
TITLE: GCN CIRCULAR
NUMBER: 9056
SUBJECT: GRB 090328B: Fermi GBM Detection
DATE: 09/03/30 18:06:00 GMT
FROM: Adam Goldstein at Fermi-GBM/UAH <adam.m.goldstein at msfc.nasa.gov>
A. Goldstein (UAH) reports on behalf of the Fermi GBM Team:
"At 17:07:04.94 UT on 28 March 2009, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 090328B (trigger 259952826 / 090328713).
The Fermi Observatory executed a maneuver following this trigger and
tracked the burst location for the next 5 hours, subject to
Earth-angle constraints.
The on-ground calculated location, using the GBM trigger
data, is RA = 155.72, DEC = +33.40 (J2000 degrees,
equivalent to 10h 23m, 33d 24'), with an uncertainty
of 7.94 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 74 degrees.
The GBM light curve consists of a single bright peak
with a duration (T90) of about 0.32 s (8-1000 keV).
The time-averaged spectrum from T0-0.13 s to T0+0.13 s is
well fit by a Band function with Epeak = 1967.0 +/- 701.0 keV,
alpha = -0.92 +/- 0.06, and beta = -2.48 +/- 0.66
(chi squared 452.6 for 482 d.o.f.).
The event fluence (8-1000 keV) in this time interval is
(9.61 +/- 0.31)E-07 erg/cm^2. The 0.064-sec peak photon flux measured
starting from T0+0.0 s in the 8-1000 keV band
is 29.83 +/- 2.38 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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