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Direct imaging of exoplanets is a challenging task that involves distinguishing faint planetary signals from the overpowering glare of their host stars, often obscured by time-varying stellar noise known as ”speckles”. The predominant algorithms for speckle noise subtraction employ principal-based point spread function (PSF) fitting techniques to discern planetary signals from stellar speckle noise. We introduce torchKLIP, a benchmark package developed within the machine learning (ML) framework PyTorch. This work enables ML techniques to utilize extensive PSF libraries to enhance direct imaging post-processing. Such advancements promise to improve the post-processing of high-contrast images from leading-edge astronomical instruments like the James Webb Space Telescope and extreme adaptive optics systems.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Chia-Lin Ko,Ewan S. Douglas, andJustin Hom
"A PyTorch benchmark for high-contrast imaging post processing", Proc. SPIE 13138, Applications of Machine Learning 2024, 1313811 (3 October 2024); https://doi.org/10.1117/12.3027407
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Chia-Lin Ko, Ewan S. Douglas, Justin Hom, "A PyTorch benchmark for high-contrast imaging post processing," Proc. SPIE 13138, Applications of Machine Learning 2024, 1313811 (3 October 2024); https://doi.org/10.1117/12.3027407