## In a nutshell

For NOEMA, create with CLIC a UV table from the current index of cross-correlation observations and selected spectral window, and read it with IMAGER

    $ clic
    CLIC> (FILE ; FIND ; SET )   ! Build your index and spectral Window selection
    CLIC> TABLE MyTable.uvt [NEW] [/MOSAIC]  !  Create a UV table
    CLIC> EXIT
    $ imager
    IMAGER> READ MyTable.uvt [/Options ]

A complete set of UV tables for all spectral windows and all sources can be automatically created from an ensemble of .hpb data files by

    $ clic
    CLIC> @ all-tables
    CLIC> EXIT
    $ imager
    IMAGER> SIC FIND *.uvt
    IMAGER> READ UV 'dir%file[1]'  ! For the first one...

For ALMA, create with CASA a list of UVFITS files from a Measuremet Set, convert them with IMAGER

    $ casa
    CASA <2>: vis='MyMeasurementSet.ms'
    CASA <3>: casagildas()
    CASA <4>: casagildas("Do")
    CASA <5>: exit()
    $ imager
    IMAGER> sic find *.uvfits
    IMAGER> for string /in dir%file
    IMAGER:   @ fits_to_uvt 'string'
    IMAGER: next

or, even simpler, by using the PIPELINE command.

    $ imager
    IMAGER> PIPELINE ORGANIZE

Conventions for file naming are described in Section . Each uv table can later be read separately.