UV_MAP Mosaics

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UV_MAP Mosaics

            [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.