Fast Holographic Deconvolution: a new technique for precision radio interferometry
Ian Sullivan, Miguel Morales, Bryna Hazelton, Wayne Arcus, David, Barnes, Gianni Bernardi, Frank Briggs, Judd D. Bowman, John Bunton, Roger, Cappallo, Brian Corey, Avinash Deshpande, Ludi deSouza, David Emrich, B. M., Gaensler, Robert Goeke, Lincoln Greenhill, David Herne

TL;DR
The paper presents Fast Holographic Deconvolution, a rapid and precise method for analyzing interferometric radio data, crucial for future cosmological observations.
Contribution
It introduces a faster deconvolution technique extending existing methods, maintaining high precision while significantly reducing computation time.
Findings
Effective and precise on MWA data
Significantly faster than existing methods
Potential impact on Epoch of Reionization studies
Abstract
We introduce the Fast Holographic Deconvolution method for analyzing interferometric radio data. Our new method is an extension of A-projection/software-holography/forward modeling analysis techniques and shares their precision deconvolution and widefield polarimetry, while being significantly faster than current implementations that use full direction-dependent antenna gains. Using data from the MWA 32 antenna prototype, we demonstrate the effectiveness and precision of our new algorithm. Fast Holographic Deconvolution may be particularly important for upcoming 21 cm cosmology observations of the Epoch of Reionization and Dark Energy where foreground subtraction is intimately related to the precision of the data reduction.
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