22.4.4 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

Argument SCAN is a special case to built a sub-catalog of spectral lines adapted to the current selection.

As post-processing (after IMAGING and TABLES), additional actions are possible

   CONTINUUM     Collect all Continuum data in one Multi-frequency set.
   SED or INDEX  Compute Spectral Index and Flux from continuum tables.
   SKY           Apply primary  beam correction to existing images.