The bandpass (in phase) of the correlator units can be calibrated
using the built-in noise source of each unit.
Cross correlation on this noise source then gives the phases
of each entry with a high signal-to-noise ratio since this input is
100% correlated. The OBS
BANDPASS command is
intended for this measurement. It automatically switches the
correlator input to the noise source, disables Walsh switching on the
first LO,
and disables delay
and phase tracking. After the measurement, the original state is
restored.
This procedure can be done while the antenna are slewing to a new pointing direction, so it introduces practically no loss of observing time when inserted at appropriate position in observing procedures. Some misfunctions of the correlators can be detected by this procedure.