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![]() TITLE: GCN CIRCULAR NUMBER: 9399 SUBJECT: GRB 090511: Fermi GBM Detection DATE: 09/05/19 20:48:51 GMT FROM: Valerie Connaughton at MSFC <valerie@nasa.gov> Valerie Connaughton (UAH) reports on behalf of the Fermi GBM Team: "At 16:25:16.37 UT on 11 May 2009, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 090511 (trigger 263751918 / 090511684).
The on-ground calculated location, using the GBM trigger
data, is RA = 161.9, DEC = 51.3 (J2000 degrees,
equivalent to 10 h 48 m, 51 d 18 '), with an uncertainty
of 7.0 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 67 degrees.
The GBM light curve consists of a single pulse
with a duration (T90) of about 14 s (8-1000 keV).
The time-averaged spectrum from T0-5.1 s to T0+4.1 s is
best fit by a power law function with an exponential
high energy cutoff. The power law index is -0.95 +/- 0.18 and
the cutoff energy, parameterized as Epeak, is 391 +/- 157 keV.
The event fluence (8-1000 keV) in this time interval is
(1.8 +/- 0.2)E-06 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+1 s in the 8-1000 keV band
is 2.5 +/- 0.4 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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