It is used in VLBI experiments, as well as spectroscopic, flux, polarisation measurements and pulsar observations. Currently receivers for frequencies 1.4–1.8 GHz, 5 GHz, 6.5 GHz, 10.8 GHz and 30 GHz are in use.
It is utilized in VLBI experiments, as well as spectroscopic, flux, polarisation measurements and pulsar observations. Currently receivers for frequencies 1.4–1.8 GHz, 5 GHz, 6.5 GHz, 10.8 GHz and 30 GHz are operational.