Direction Dependent Corrections in Polarimetric Radio Imaging II: A-Solver Methodology A low-order solver for the A-Term of the A-Projection algorithm
Preshanth Jagannathan, S. Bhatnagar, W. Brisken, A.R. Taylor

TL;DR
This paper introduces the A-Solver methodology, combining physical modeling and optimization, to accurately model the antenna aperture illumination pattern for improved radio interferometric imaging.
Contribution
It presents a low-order, physically motivated model for the antenna A-term that enhances correction accuracy in wide-bandwidth radio imaging.
Findings
The A-Solver captures dominant frequency-dependent antenna effects.
The methodology improves sensitivity and imaging performance.
The approach is adaptable to different antenna types.
Abstract
The effects of the antenna far-field power pattern limits the imaging performance of modern wide-bandwidth, high-sensitivity interferometric radio telescopes. Given a model for the aperture illumination pattern (AIP) of the antenna, referred to as the A-term, the wide-band (WB) A-Projection algorithm corrects for the effects of its time, frequency, and polarization structure. The level to which this correction is possible depends on how accurately the A-term, represents the true AIP. In this paper, we describe the A-Solver methodology that combines physical modeling with optimization to holographic measurements to build an accurate model for the AIP. Using a parametrized ray-tracing code as the predictor, we solve for the frequency dependence of the antenna optics and show that the resulting low-order model for the Karl G. Jansky Very Large Array (VLA) antenna captures the dominant…
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