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