[vsnet-grb-info 15509] GRB 140907A: Fermi GBM Detection
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Sep 9 00:32:49 JST 2014
TITLE: GCN CIRCULAR
NUMBER: 16798
SUBJECT: GRB 140907A: Fermi GBM Detection
DATE: 14/09/08 15:32:05 GMT
FROM: Binbin Zhang at UAH <binbin.zhang at uah.edu>
Bin-Bin Zhang (UAH) reports on behalf of the Fermi GBM Team:
"At 16:07:11.80 UT on 07 September 2014, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 140907A (trigger 431798834 / 140907672), which
was also detected by the Swift/BAT (Krimm et al 2014, GCN 16788)
The GBM on-ground location is consistent with the Swift position.
The angle from the Fermi LAT boresight is 16 degrees.
The GBM light curve consists of a single pulse with multiple peaks.
The total duration (T90) is about 35 +/- 10 s (50-300 keV).
The time-averaged spectrum from T0-12 s to T0+22 s is
best fit by a power law function with an exponential
high-energy cutoff. Â The power law index is -0.97 +/- 0.08 Â and
the cutoff energy, parameterized as Epeak, is 113 +/- 7 keV.
The event fluence (10-1000 keV) in this time interval is
(5.5 +/- 0.2)E-06 erg/cm^2. The 1.024-sec peak photon flux measured
starting from T0+8.9 s in the 10-1000 keV band
is 4.2 +/- 0.3 Â 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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