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[ascl:2205.014] FHD: Fast Holographic Deconvolution

FHD is an open-source imaging algorithm for radio interferometers and is written in IDL. The three main use-cases for FHD are efficient image deconvolution for general radio astronomy, fast-mode Epoch of Reionization analysis, and simulation. FHD inputs beam models, calibration files, and sky model catalogs and requires input data to be in uvfits format.

Code site:
https://github.com/EoRImaging/FHD
Described in:
https://ui.adsabs.harvard.edu/abs/2012ApJ...759...17S https://ui.adsabs.harvard.edu/abs/2019PASA...36...26B https://ui.adsabs.harvard.edu/abs/2022PASA...39...23B
Bibcode:
2022ascl.soft05014S

Views: 1462

ascl:2205.014
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