Fast gain calibration in radio astronomy using alternating direction implicit methods: Analysis and applications
Stefano Salvini, Stefan J. Wijnholds

TL;DR
This paper introduces an efficient ADI-based gain calibration method for large radio arrays, demonstrating its convergence, near-optimal performance, and successful application in LOFAR pipelines, significantly reducing computational complexity.
Contribution
The paper presents a new ADI algorithm for gain calibration that converges to the optimal solution and reduces complexity from O(P^3) to O(P^2), with proven performance and practical application.
Findings
Algorithm confirms O(P^2) complexity and excellent numerical properties.
Performs near the Cramer-Rao bound in simulations.
Achieves an order-of-magnitude speedup in LOFAR data calibration.
Abstract
Context. Modern radio astronomical arrays have (or will have) more than one order of magnitude more receivers than classical synthesis arrays, such as the VLA and the WSRT. This makes gain calibration a computationally demanding task. Several alternating direction implicit (ADI) approaches have therefore been proposed that reduce numerical complexity for this task from to , where is the number of receive paths to be calibrated. Aims. We present an ADI method, show that it converges to the optimal solution, and assess its numerical, computational and statistical performance. We also discuss its suitability for application in self-calibration and report on its successful application in LOFAR standard pipelines. Methods. Convergence is proved by rigorous mathematical analysis using a contraction mapping. Its numerical, algorithmic, and…
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