Next: Skydips and determination of
Up: Single-dish calibration in a
Previous: Description of the received
Contents
In order to disentangle the different effects, three steps are needed
- Once in a while, skydips are measured to determine the telescope
forward efficiency (
) as a function of frequency;
- Every 10 to 15 minutes, observations of 1) two references at very
different temperatures (the hot and cold load) and 2) the atmosphere in a
direction devoid of signal are used to deduce the opacity of the
atmosphere and the calibration factor. In modern system, the hot load is
a foam at roughly the room temperature and the cold load is the cryostat
window of the receiver which is roughly at liquid nitrogen temperature;
- The telescope is regularly switched on and off source to subtract the
atmospheric contribution to the signal seen by the receiver.
Subsections
Gildas manager
2014-07-01