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![]() TITLE: GCN CIRCULAR NUMBER: 9413 SUBJECT: GRB 090516B: Fermi GBM detection DATE: 09/05/20 17:04:52 GMT FROM: Sheila McBreen at MPE <smcbreen@mpe.mpg.de> Sheila McBreen (UCD/MPE) reports on behalf of the Fermi GBM Team: "At 03:17:20.17 UT on 16 May 2009, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 090516B (trigger 264136642 / 090516137).
The on-ground calculated location, using the GBM trigger
data, is RA = 122.2, DEC = -71.62 (J2000 degrees,
equivalent to 08 h 09 m, -71 d 37 '), with an uncertainty
of 2.6 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 45 degrees.
The GBM light curve consists of several overlapping
peaks from the trigger to about 140 s and possible
weak emission out to about 350 s.
The time-averaged spectrum from T0 s to T0+138 s is
adequately fit by a power law function with an exponential
high energy cutoff. The power law index is -1.01 (+/-0.06) and
the cutoff energy, parameterized as Epeak, is
327.0 (+/-58.7) keV (chi squared 419 for 359 d.o.f.).
The event fluence (8-1000 keV) in this time interval is
(3.0 +/- 0.1)E-05 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+80 s in the 8-1000 keV band
is 4.0 +/- 0.2 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
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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