Skip to main content
Testing. You are viewing the public testing version of GCN. For the production version, go to https://gcn.nasa.gov.
Introducing Einstein Probe, Astro Flavored Markdown, and Notices Schema v4.0.0. See news and announcements

GCN Circular 2946

Subject
SGR 1806-20: Further VLA Observations
Date
2005-01-10T15:10:43Z (20 years ago)
From
Patrick B. Cameron at Caltech <pbc@astro.caltech.edu>
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 10.60 UT.

We find the following preliminary flux densities:

Freq (GHz)    Flux density (mJy)
--------------------------------
8.46	       8 +/- 1


The National Radio Astronomy Observatory is operated by Associated
Universities, Inc., under cooperative agreement with the National Science
Foundation."


--------------------------------------
P. Brian Cameron
Caltech Astrophysics
Phone: (626) 395-6857
Questions or comments?
Contact GCN directly.
Have you found a bug in GCN?
Open an issue.
Want to contribute code to GCN?
Get involved on GitHub.

gcn.nasa.gov

A service of the Astrophysics Science Division at NASA Goddard Space Flight Center

Looking for U.S. government information and services? Visit USA.gov