Next: 7.2.4 Side band calibration
Up: 7.2 Bandpass calibration
Previous: 7.2.2 IF passband calibration
Subsections
To actually determine the functions
we observe a strong source,
with a frequency-independent visibility.
The visibilities are
|
(7.14) |
Then
|
(7.15) |
since the frequency independent factors cancel out in the right-end
side. One then averages the measurements on a time long enough to
get a decent signal-to-noise ratio. One solves for the
antenna-based coefficients in both amplitude and phase; then
polynomial amplitude and phase passband curves are fitted to the
data.
The passband calibrated visibility data will then be:
|
(7.16) |
the amplitude and phase of which should be flat functions of frequency.
The most important here is the
phase precision: it sets the uncertainty for relative positions of
spectral features in the map. A rule of thumb is:
|
(7.17) |
where
is the synthesized beam, and
the
relative position uncertainty. The signal to noise ratio on the
bandpass calibration should be better than the signal to noise
ration of the spectral features observed; otherwise the relative
positional accuracy will be limited by the accuracy of the passband
calibration.
The amplitude accuracy can be very important too, for instance when
one wants to measure a weak line in front of a strong continuum, in
particular for a broad line. In that case one needs to measure the
passband with an amplitude accuracy better than that is needed on
source to get desired signal to noise ratio. Example: we want to
measure a line which is of the continuum, with a SNR of 20 on
the line strength; then the SNR on the continuum source should be
200, and the SNR on the passband calibration should be at least as
good.
Next: 7.2.4 Side band calibration
Up: 7.2 Bandpass calibration
Previous: 7.2.2 IF passband calibration
S.Guilloteau
2000-01-19