Efficient deconvolution methods for astronomical imaging: algorithms and IDL-GPU codes
M. Prato, R. Cavicchioli, L. Zanni, P. Boccacci, M. Bertero

TL;DR
This paper introduces accelerated deconvolution algorithms for astronomical imaging using scaled gradient projection methods, implemented in IDL-GPU, significantly improving efficiency over traditional Richardson-Lucy methods.
Contribution
It applies scaled gradient projection to astronomical deconvolution problems and implements GPU acceleration, achieving substantial speedups over classical methods.
Findings
Speedup factors range from 4 to over 30 compared to Richardson-Lucy.
GPU implementation yields up to two orders of magnitude acceleration.
Algorithms effectively handle single, multiple image deconvolution, and boundary correction.
Abstract
The Richardson-Lucy method is the most popular deconvolution method in astronomy because it preserves the number of counts and the non-negativity of the original object. Regularization is, in general, obtained by an early stopping of Richardson-Lucy iterations. In the case of point-wise objects such as binaries or open star clusters, iterations can be pushed to convergence. However, it is well-known that Richardson-Lucy is an inefficient method. In most cases, acceptable solutions are obtained at the cost of hundreds or thousands of iterations. A general optimization method, referred to as the scaled gradient projection method, has been proposed for the constrained minimization of continuously differentiable convex functions. It is applicable to the non-negative minimization of the Kullback-Leibler divergence. If the scaling suggested by Richardson-Lucy is used in this method, then it…
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