The content discusses the challenges of deconvolving astronomical images due to beam effects, proposing an unsupervised network architecture incorporating prior physical knowledge. It explores various regression networks and loss functions, emphasizing the importance of eliminating beam distortions for precise analysis.
The study compares different deconvolution methods, highlighting the effectiveness of the proposed PI-AstroDeconv approach. It details the network architecture, FFT-accelerated convolution, and selection of appropriate loss functions. The experiments demonstrate significant improvements in image quality and restoration using the proposed method.
Furthermore, future research directions include exploring alternative networks like Vision Transformer and applying the model to various telescopes for enhanced image quality and broader astronomical studies.
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by Shulei Ni,Yi... klokken arxiv.org 03-05-2024
https://arxiv.org/pdf/2403.01692.pdfDypere Spørsmål