SCAN

          IMAGER\PIPELINE SCAN

        Scan  the  currently  selected  UV  tables (from All%FIlter) to find out
    which spectral lines from the current catalog are covered by  the  available
    spectral  setups.  The  identified  lines are stored in a new local catalog,
    named

      local-coverage.lin

    Lines may appear several times in this catalog, as the UV  tables  may  have
    redundant  spectral coverage.  A trimmed version, ordered by increasing fre-
    quency, is also created in

      sorted-coverage.lin

    It can be re-used after edition as a local catalog. Both catalogs are in  an
    Astro  CSV  (Comma  Separated Value) format and are easily editable (e.g. to
    suppress spectral lines too close to each other, in particular for hyperfine
    component groups).

        This is Step 2.4, NEXT step is ChECK.