Spillover can double T
at L-band when observing sources at
low elevation. Since data obtained at lower elevations will therefore
be noisier, the observer may wish to down-weight them relative to the
parts of the run at which the object under study was at higher
elevations. Unfortunately, there is no easy way to do this in AIPS;
the task WTMOD offers only limited flexibility to modifying
weights. The best option is to avoid observing below elevations of
about 30
. Some objects, such as the Galactic center, never
reach high elevations. For those situations one has to take the higher
system temperature into account when estimating the rms noise which
one aims to achieve.