[CLEAN\]PRIMARY [BeamSize] [/TRUNCATE Percent]
Apply approximate primary beam correction to a single field deconvolved
(CLEAN) image, in order to create the sky brightness image (named SKY).
The truncation level is given by default by variable CLEAN_TRUNCATE, and
can be overriden by the /TRUNCATE option.
The primary beam model is a simple Gaussian. If BeamSize (in radian) is
specified, uses the corresponding half-power beam size to determine the
Gaussian beam. If not, the parameters are taken from the telescope pa-
rameters, as found in the telescope section of the CLEAN image and the
observing frequency from the CLEAN image (e.g. for ALMA it uses 1.13
Lambda/D).
The SKY image is written with extension .lmv-sky by command WRITE.
Subsections
Gildas manager
2023-06-01