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GCN Circular 2948

Subject
SGR 1806-20: Further VLA Observations
Date
2005-01-13T20:20:42Z (21 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."
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