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Generalized Recorrupted-to-Recorrupted: Self-Supervised Learning Beyond Gaussian Noise

CVPR 2025 · Label-efficient and robust learning › Self-supervised and contrastive · approach: Pretext-task visual pre-training · 7 citations (OpenAlex)

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Extends self-supervised Recorrupted-to-Recorrupted (R2R) to non-Gaussian additive noise and natural exponential family noise (Poisson, Gamma, Binomial) by generating independent noisy pairs, yielding an unbiased supervised-equivalent MSE/NLL loss that recovers SURE as a special case.

Problem

Self-supervised image restoration from noisy measurements alone is well established for Gaussian noise (R2R, SURE), but its effectiveness for non-Gaussian additive noise and exponential-family noise such as Poisson and Gamma is unexplored.

Approach

Recorrupt each noisy measurement into two conditionally independent noisy versions via a noise-distribution-specific splitting (y = (1-α)y1 + αy2), so that a simple MSE or negative-log-likelihood loss on (y1, y2) is an unbiased estimator of the supervised loss; as α→0 it reduces to a SURE-type loss without computing divergences.

Key results

Measured effects reported in the paper

What was changedWhereMeasuredEffect
Add GR2R recorruption with third-order moment matching instead of standard R2R second-moment matching (ablation)R2R on DIV2K log-Rayleigh denoising · Additive log-Rayleigh noisePSNR: 25.32 ± 0.79 -> 29.93 ± 1.50Helped
Use GR2R-NLL rather than GR2R-MSE (ablation)GR2R on DIV2K Poisson denoising · Poisson noise, γ=0.5PSNR: 24.69 -> 25.07Helped
Use GR2R-MSE rather than GR2R-NLL (ablation)GR2R on DIV2K Poisson denoising · Poisson noise, γ=0.01PSNR: 33.90 -> 33.92No clear effect
Use GR2R-MSE rather than GR2R-NLL (ablation)GR2R on SAR Gamma denoising · Gamma noise, ℓ=30PSNR: 30.43 -> 31.58Helped
Use GR2R-MSE rather than GR2R-NLL (ablation)GR2R on SAR Gamma denoising · Gamma noise, ℓ=1PSNR: 22.19 -> 22.38No clear effect
Train with GR2R rather than Noise2ScoreImage denoising on fastMRI · Gaussian noise, σ=0.05PSNR: 34.42 -> 35.38Helped
Train with GR2R rather than SUREImage denoising on fastMRI · Gaussian noise, σ=0.05PSNR: 35.31 -> 35.38No clear effect
Train with GR2R rather than supervised MSEImage denoising on fastMRI · Gaussian noise, σ=0.05PSNR: 35.41 -> 35.38No clear effect
Train with GR2R-MSE rather than Neigh2NeighSAR Gamma denoising · Gamma noise, ℓ=30PSNR: 30.34 -> 31.58Helped
Train with GR2R-NLL rather than Neigh2NeighDIV2K Poisson denoising · Poisson noise, γ=0.5PSNR: 24.90 -> 25.07Helped

Surprising findings

Limitations

Experimental setup

Datasets: DIV2K SAR Image Despeckling dataset fastMRI

Benchmarks: DIV2K SAR Image Despeckling dataset fastMRI

Metrics: PSNR SSIM

Baselines: R2R SURE PURE Neigh2Neigh Noise2Score Equivariant Imaging Supervised MSE

Builds on: Recorrupted-to-Recorrupted (R2R) Stein's unbiased risk estimator (SURE) Noise2Noise Equivariant Imaging GSURE

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