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- APCLN : Clark CLEAN of dirty image.
- BSMAP : Bi-Spectrum imaging of simple, weak objects.
- HBCLN : Högbom CLEAN of dirty image.
- HORUS : Fourier transform visibilties to dirty image directly from
multi-source file
- IMERG : Merges high and low res. images.
- LTESS : Make linear combination mosaics.
- MX : Fourier transform visibilties to dirty image and CLEAN
- RSTOR : Restores a CC file to an image with a gaussian beam.
- SDCLN : SDI CLEAN of dirty image
- UVIMG : Grid UV data into an "image".
- UVMAP : Fourier transform visibilties to dirty image
- UTESS : Maximum Entropy deconvolution of dirty image that does
not enforce positivity. Good for Stokes Q, U, and V.
- VTESS : Maximum Entropy deconvolution of dirty image
nkilleen@atnf.csiro.au