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Published November 6, 2023 | Published
Journal Article

Discovering Structure From Corruption for Unsupervised Image Reconstruction

  • 1. ROR icon California Institute of Technology

Abstract

We consider solving ill-posed imaging inverse problems without access to an image prior or ground-truth examples. An overarching challenge in these inverse problems is that an infinite number of images, including many that are implausible, are consistent with the observed measurements. Thus, image priors are required to reduce the space of possible solutions to more desirable reconstructions. However, in many applications it is difficult or potentially impossible to obtain example images to construct an image prior. Hence inaccurate priors are often used, which inevitably result in biased solutions. Rather than solving an inverse problem using priors that encode the spatial structure of any one image, we propose to solve a set of inverse problems jointly by incorporating prior constraints on the collective structure of the underlying images. The key assumption of our work is that the underlying images we aim to reconstruct share common, low-dimensional structure. We show that such a set of inverse problems can be solved simultaneously without the use of a spatial image prior by instead inferring a shared image generator with a low-dimensional latent space. The parameters of the generator and latent embeddings are found by maximizing a proxy for the Evidence Lower Bound (ELBO). Once identified, the generator and latent embeddings can be combined to provide reconstructed images for each inverse problem. The framework we propose can handle general forward model corruptions, and we show that measurements derived from only a small number of ground-truth images ( 150 ) are sufficient for image reconstruction. We demonstrate our approach on a variety of convex and non-convex inverse problems, including denoising, phase retrieval, and black hole video reconstruction.

Copyright and License

© 2023 IEEE.

Acknowledgement

The authors would like to thank Ben Prather, Abhishek Joshi, Vedant Dhruv, Chi-kwan Chan, and Charles Gammie for providing black hole simulations used in this work. We would also like to thank Aviad Levis, Yu Sun, and Jorio Cocola for their feedback and guidance.

Funding

This work was supported in part by the Jet Propulsion Laboratory and Caltech under a contract with the National Aeronautics and Space Administration and funded through the PDRDF in part by NSF under Awards 2048237 and 1935980, and in part by Amazon AI4Science Partnership Discovery Grant.

Contributions

Oscar Leong and Angela F. Gao contributed equally to this work.

Additional details

Created:
May 6, 2024
Modified:
May 6, 2024