GCN Circular 2935
Subject
Third epoch observations of SGR 1806-20 with VLA
Date
2005-01-05T16:16:11Z (19 years ago)
From
Chryssa Kouveliotou at MSFC <chryssa.kouveliotou-1@nasa.gov>
B. M. Gaensler (CfA), C. Kouveliotou (NASA/MSFC, NSSTC), J. Gelfand (CfA),
R. Wijers (U. Amsterdam), M. Garrett (JIVE), M. Finger, P. Woods, S. Patel (USRA,
NSSTC), M. McLaughlin (Jodrell Bank), R. Fender (U. Southampton),
T. Delaney (CfA) report on behalf of a larger team:
We observed the soft gamma-ray repeater SGR 1806-20 with the Very Large
Array (VLA) in the A-configuration for a third time on January 5, 2005
for one hour (mean epoch approx 1600 UT). (See GCN #2928, #2929, #2933;
ATEL #373, #375 for earlier results).
Preliminary flux levels for 2005-Jan-05.66 are as follows:
4.9 GHz: 57(2) mJy
8.5 GHz: 31(2) mJy
The source continues to fade, but at a slower rate consistent with a power law of
index -1.6(2) at 4.9 GHz. Further observations will take place on January 6.