Korean VLBI Network (KVN)
Antenna Pointing Accuracy
A sample of late type stars
has been used continuously
to maintain the pointing accuracy of the telescope during 2009-2014.
The following table describes the accuracies of pointing models
established for three KVN radio telescopes in 2015.
The root mean square (rms) of the residual pointing offsets
between the observations and the pointing models are listed
in total, azimuth, and elevation,
respectively, for each epoch and telescope.
|Yonsei||4.0||2.0||3.5||43 GHz||2015.03.09 |
|Tamna ||6.0||3.3||5.0||43 GHz||2015.03.09|
In case of observations during a daytime, especially at sunrise and sunset,
the pointing observations must be conducted out at least every hour
for maintaining the pointing accuracy to be less than 6 arcseconds in rms.
The residual of pointing model measured at KVNYS.
The residual of pointing model measured at KVNUS.
The residual of pointing model measured at KVNTN.