[vsnet-grb-info 6961] Fermi GBM detection of a weak source
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Sun Nov 23 03:04:28 JST 2008
TITLE: GCN CIRCULAR
NUMBER: 8545
SUBJECT: Fermi GBM detection of a weak source
DATE: 08/11/22 18:04:14 GMT
FROM: Rob Preece at UAH <Rob.Preece at nasa.gov>
Rob Preece (UAH) and Alexander van der Horst (NASA/MFSC/ORAU) report
on behalf of the Fermi GBM Team:
"At 21:22:28.14 UT on 15 November 2008, the Fermi Gamma-ray Burst
Monitor
(GBM) triggered and located a weak source (trigger 248476949 /
081115.891).
The most likely nature of the source is a GRB, but it could also be
Cygnus
X-1. Since the source is very weak, it is not possible to find a
reliable
on-ground calculated location and to perform any spectral analysis."
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