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Deep Probabilistic Imaging: Uncertainty Quantification and Multi-modal Solution Characterization for Computational Imaging

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arxiv 2010.14462 v2 pith:DSCGHRCT submitted 2020-10-27 cs.LG astro-ph.IMcs.CVeess.IVeess.SP

classification cs.LGastro-ph.IMcs.CVeess.IVeess.SP
keywords imagingdeepimageapproachdataprobabilisticuncertaintycomputational
verification ladder T0 review T1 audit T2 compute T3 formal

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Computational image reconstruction algorithms generally produce a single image without any measure of uncertainty or confidence. Regularized Maximum Likelihood (RML) and feed-forward deep learning approaches for inverse problems typically focus on recovering a point estimate. This is a serious limitation when working with underdetermined imaging systems, where it is conceivable that multiple image modes would be consistent with the measured data. Characterizing the space of probable images that explain the observational data is therefore crucial. In this paper, we propose a variational deep probabilistic imaging approach to quantify reconstruction uncertainty. Deep Probabilistic Imaging (DPI) employs an untrained deep generative model to estimate a posterior distribution of an unobserved image. This approach does not require any training data; instead, it optimizes the weights of a neural network to generate image samples that fit a particular measurement dataset. Once the network weights have been learned, the posterior distribution can be efficiently sampled. We demonstrate this approach in the context of interferometric radio imaging, which is used for black hole imaging with the Event Horizon Telescope, and compressed sensing Magnetic Resonance Imaging (MRI).

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Cited by 2 Pith papers

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  1. Deep Learning VLBI Image Reconstruction with Closure Invariants

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    A transformer-based deep learning network reconstructs VLBI images directly from closure invariants, achieving median NXCORR fidelity above 0.9 on untrained synthetic morphologies.

  2. Deep learning inference with the Event Horizon Telescope II. The Zingularity framework for Bayesian artificial neural networks

    astro-ph.IM 2025-06 conditional novelty 5.0 of 10

    Bayesian neural networks trained on synthetic EHT observations of Sgr A* and M87* recover spin and magnetic state well in cross-code tests, but give overconfident wrong estimates for temperature ratio and inclination ...

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