PIPELINE Arguments:

            PIPELINE  supports  the  following arguments when not used in Widget
    mode, given here in sequential order of actions
      ORGANIZE      Prepare the UV tables and directory layout
      SETUP         Basic setup, composed of the 4 following sub-steps:
        FIND          Locate the UV tables
        SELECT        Select the Wide bands vs Narrow bands
        EXPLORE       Explore imaging parameters
        SCAN          Explore covered spectral lines
      CHECK         Check if Self-Calibration is possible
      COMPUTE (or SELF)   Compute Self-calibration
      COLLECT       Collect all Self-calibration solutions
      APPLY         Apply Self-calibration
      TIME          Time average to gain space
      TABLES        Create per-line UV tables
      IMAGE         Image all data
      SHOW          Show self-calibration results
      SAVE          Save parameters
    In addition argument SKY can be used to apply primary   beam  correction  to
    existing  images.  Argument SCAN is a special case to built a sub-catalog of
    spectral lines adapted to the current selection.