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![]() TITLE: GCN CIRCULAR NUMBER: 10397 SUBJECT: GRB 100205B: Fermi GBM detection DATE: 10/02/07 18:20:33 GMT FROM: David Gruber at MPE <dgruber@mpe.mpg.de> David Gruber (MPE) reports on behalf of the Fermi GBM Team: "At 11:45:38.26 UT on 05 February 2010, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 100205B (trigger 287063140 / 100205490).
The on-ground calculated location, using the GBM trigger
data, is RA = 133.9, DEC = -23.0 (J2000 degrees,
equivalent to 08h 55m, 23d 00'), with an uncertainty
of 8.2 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 102 degrees.
The GBM light curve consists of a single pulse
with a duration (T90) of about 13.6 +/- 1.6s (8-1000 keV).
The time-averaged spectrum from T0-1.024s to T0+7.168 s is
best fit by a power law function with an exponential
high energy cutoff. The power law index is -0.47 (+0.20/-0.19) and
the cutoff energy, parameterized as Epeak, is 124.20 (+16.0/-12.2)keV
(c-stat 468.61 for 349 d.o.f.).
The event fluence (8-1000 keV) in this time interval is
(1.410 +/- 0.082)E-6 erg/cm^2. The 1.024-sec peak photon flux measured
starting from T0 in the 8-1000 keV band
is 2.98 +/- 0.22 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
This site was created by Robert Quimby
Database maintained by Robert Quimby, Erin McMahon, and Jeremy Murphy Information displayed on this site is compiled from GCN Circulars and other sources as indicated. |
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