PolyCLEAN: Atomic optimization for super-resolution imaging and uncertainty estimation in radio interferometry

Context . Imaging in radio interferometry requires solving an ill-posed noisy inverse problem, for which the most adopted algorithm is the original CLEAN algorithm and its variants. Alternative explicit optimization methods have gained increasing attention, as they demonstrate excellent reconstruction quality thanks to their ability to enforce Bayesian priors. Nowadays, the main limitation to their adoption is run-time speed. Additionally, uncertainty quantification is difficult for both CLEAN and convex optimization techniques. Aims . We address two issues for the adoption of convex optimization in radio interferometric imaging. First, we propose a method for a fine resolution setup, which scales naturally in terms of memory usage and reconstruction speed. Second, we develop a new tool to localize a region of uncertainty, paving the way for quantitative imaging in radio interferometry. Methods . The classical ℓ 1 penalty is used to turn the inverse problem into a sparsity-promoting optimization. For efficient implementation, the so-called Frank-Wolfe algorithm is used together with a polyatomic refinement. The algorithm naturally produces sparse images at each iteration, leveraged to reduce memory and computational requirements. In that regard, PolyCLEAN reproduces the numerical behavior of CLEAN, while guaranteeing that it solves the minimization problem of interest. Additionally, we introduce the concept of the dual certificate image, which appears as a numerical byproduct of the Frank-Wolfe algorithm. This image is proposed as a tool for uncertainty quantification on the location of the recovered sources. Results . PolyCLEAN demonstrates good scalability performance, in particular for fine-resolution grids. On simulations, the Pythonbased implementation is competitive with the fast numerically-optimized CLEAN solver. This acceleration does not affect image reconstruction quality: PolyCLEAN images are consistent with CLEAN-obtained ones for both point sources and diffuse emission recovery. We also highlight PolyCLEAN reconstruction capabilities on observed radio measurements. Conclusions . PolyCLEAN can be considered as an alternative to CLEAN in the radio interferometric imaging pipeline, as it enables the use of Bayesian priors without impacting the scalability and numerical performance of the imaging method.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2024-12-11
DOI
https://doi.org/10.1051/0004-6361/202450970
Citations
5
Primary Topic
Medical Imaging Techniques and Applications
Type
article
Field-Weighted Citation Impact
2.02

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article

PolyCLEAN: Atomic optimization for super-resolution imaging and uncertainty estimation in radio interferometry

Sepand Kashani, Julien Fageot, Adrian Jarret, Matthieu Simeoni et al.
5 citations
Astronomy and Astrophysics
Medical Imaging Techniques and Applications
2.02
article

PolyCLEAN: Atomic optimization for super-resolution imaging and uncertainty estimation in radio interferometry

Sepand Kashani, Julien Fageot, Adrian Jarret, Matthieu Simeoni, Paul Kennedy Hurley, Joan Rué‐Queralt
article en
5 citations

Abstract

Context . Imaging in radio interferometry requires solving an ill-posed noisy inverse problem, for which the most adopted algorithm is the original CLEAN algorithm and its variants. Alternative explicit optimization methods have gained increasing attention, as they demonstrate excellent reconstruction quality thanks to their ability to enforce Bayesian priors. Nowadays, the main limitation to their adoption is run-time speed. Additionally, uncertainty quantification is difficult for both CLEAN and convex optimization techniques. Aims . We address two issues for the adoption of convex optimization in radio interferometric imaging. First, we propose a method for a fine resolution setup, which scales naturally in terms of memory usage and reconstruction speed. Second, we develop a new tool to localize a region of uncertainty, paving the way for quantitative imaging in radio interferometry. Methods . The classical ℓ 1 penalty is used to turn the inverse problem into a sparsity-promoting optimization. For efficient implementation, the so-called Frank-Wolfe algorithm is used together with a polyatomic refinement. The algorithm naturally produces sparse images at each iteration, leveraged to reduce memory and computational requirements. In that regard, PolyCLEAN reproduces the numerical behavior of CLEAN, while guaranteeing that it solves the minimization problem of interest. Additionally, we introduce the concept of the dual certificate image, which appears as a numerical byproduct of the Frank-Wolfe algorithm. This image is proposed as a tool for uncertainty quantification on the location of the recovered sources. Results . PolyCLEAN demonstrates good scalability performance, in particular for fine-resolution grids. On simulations, the Pythonbased implementation is competitive with the fast numerically-optimized CLEAN solver. This acceleration does not affect image reconstruction quality: PolyCLEAN images are consistent with CLEAN-obtained ones for both point sources and diffuse emission recovery. We also highlight PolyCLEAN reconstruction capabilities on observed radio measurements. Conclusions . PolyCLEAN can be considered as an alternative to CLEAN in the radio interferometric imaging pipeline, as it enables the use of Bayesian priors without impacting the scalability and numerical performance of the imaging method.

Astronomy and AstrophysicsVol. 693
National Audiovisual Institute (PL), École Polytechnique Fédérale de Lausanne (CH), Western Sydney University (AU)
National Science Foundation, École Polytechnique Fédérale de Lausanne, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
Industry, innovation and infrastructure
Openalex Percentile: Top 12%
Medical Imaging Techniques and Applications
2.02
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