GCN Circular 2948
Subject
SGR 1806-20: Further VLA Observations
Date
2005-01-13T20:20:42Z (19 years ago)
From
Patrick B. Cameron at Caltech <pbc@astro.caltech.edu>
On Mon, 10 Jan 2005, P Brian Cameron wrote:
P. B. Cameron (Caltech) and S. R. Kulkarni (Caltech) report:
"We observed the soft gamma-ray repeater SGR 1806-20
with the Very Large Array (VLA) in A-configuration on 2005
Jan 13.8 UT.
We find the following preliminary flux densities:
Freq (GHz) Flux density (mJy)
--------------------------------
8.46 5.3 +/- 0.4
The National Radio Astronomy Observatory is operated by Associated
Universities, Inc., under cooperative agreement with the National Science
Foundation."