[vsnet-grb-info 7868] GRB 090519B: Fermi GBM detection
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Thu May 21 00:33:04 JST 2009
TITLE: GCN CIRCULAR
NUMBER: 9412
SUBJECT: GRB 090519B: Fermi GBM detection
DATE: 09/05/20 15:32:50 GMT
FROM: Andreas von Kienlin at MPE <azk at mpe.mpg.de>
A. von Kienlin (MPE) reports on behalf of the Fermi GBM Team:
"At 11:05:27.54 UT on 19 May 2009, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 090519B (trigger 264423929 / 090519462).
The on-ground calculated location, using the GBM trigger
data, is RA = 105.9, DEC = -56.7 (J2000 degrees,
equivalent to 07h 04m, 56d 42'), with an uncertainty
of 3.9 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 18 degrees.
The GBM light curve shows a single peak lasting
about 4 seconds superimposed on a lower-level continuum.
The burst duration (T90) is about 87 s (8-1000 keV).
The time-averaged spectrum from T0-2.432 s to T0+1.152 s is
well fit by a simple power law function with index -1.63 +/- 0.05
(chi squared 822 for 720 d.o.f.).
The event fluence (8-1000 keV) in this time interval is
(1.40 +/- 0.01)E-06 erg/cm^2. The 1-sec peak photon flux measured
starting from T0-0.640 s in the 8-1000 keV band
is 5.02 +/- 0.14 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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