
\command{POINTING} observations are done to optimize the positioning of the
telescope in Azimuth and Elevation. This is normally done by continuum
observations of a cross scan in azimuth and elevation on a point
source (or at least a small source) near the intended target source.

It is normally used with \swb\ or \sww; 
it is also possible with \total. 
(With the bolometer \pointing\ is done with \sww).

A calibration is not needed for \pointing, if one is only interested
in the pointing corrections, and not in the source intensity.

After a pointing the data processing software displays the results
and you can enter a correction for the observed pointing offsets 
with the command

\command{SET POINTING azimuthCorrection elevationCorrection}

Note that this is the total correction, i.e., the previous correction
plus the additional offset found with the \command{POINTING} observation.

\input{inc/pakoIncSavePointing.tex}
