[vsnet-grb-info 8183] GRB 090711: Fermi GBM detection
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Mon Jul 27 23:10:19 JST 2009
TITLE: GCN CIRCULAR
NUMBER: 9713
SUBJECT: GRB 090711: Fermi GBM detection
DATE: 09/07/27 14:10:00 GMT
FROM: Bill Paciesas at UAH <bill.paciesas at nasa.gov>
Colleen A. Wilson-Hodge (NASA/MSFC)
reports on behalf of the Fermi GBM Team:
"At 20:23:22.92 UT on 11 July 2009, the Fermi Gamma-Ray Burst Monitor
triggered and located GRB 090711 (trigger 269036604 / 090711850).
The on-ground calculated location, using the GBM trigger
data, is RA = 139.6, DEC = -64.7 (J2000 degrees,
equivalent to 09 h 18 m, -64 d 42 '), with an uncertainty
of 1 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 13 degrees.
The GBM light curve consists of multiple peaks
with a duration of at least 100 s (8-1000 keV). The GBM detectors
were turned off for SAA entry about 83 seconds after the
trigger. The time-averaged spectrum from T0-20.992 s to T0+82.433 s is
adequately fit by a power law function with an exponential
high energy cutoff. The power law index is 1.3 +/- 0.1 and
the cutoff energy, parameterized as Epeak, is 210 +/- 70 keV
The event fluence (8-1000 keV) in this time interval is
(1.17 +/- 0.16 )E-05 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+1.536 s in the 8-1000 keV band
is 4.2 +/- 0.6 ph/s/cm^2.
The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."
More information about the vsnet-grb-info
mailing list