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 employed in VLBI experiments, spectroscopic, flux, polarisation measurements, and pulsar observations. Receivers for frequencies ranging from 1.4 to 1.8 GHz, 5 GHz, 6.5 GHz, 10.8 GHz, and 30 GHz are currently being used.