[CLEAN\]UV_MAP [[CenterX CenterY Unit] [ANGLE AngleValue]
/FIELDS FieldList [/TRUNCATE Percent]
The UV data can be a Mosaic UV table. In this case, UV_MAP will image
the Mosaic, using appropriate primary beam size and truncation level.
By default, the primary beam size is taken from the telescope parame-
ters, either as found in the telescope section of the UV table and the
observing frequency (e.g. for ALMA it uses 1.13 Lambda/D). If absent,
the telescope section information can be added by command SPECIFY TELE-
SCOPE.
The truncation level for individual pointings is taken from variable
MAP_TRUNCATE or from the /TRUNCATE option argument. It should be 0 for
high dynamic range. Non zero values may be used with caution in case of
large pointing errors.
Gildas manager
2023-06-01