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REVIEW 3 major objections 6 minor 56 references

Image Restoration Learning via Noisy Supervision in the Fourier Domain

T0 review · 3 major / 6 minor · reviewed 2026-08-07 · deepseek-v4-flash

Pith's one-line read Training with one noisy target per scene reproduces clean-target training when the loss is computed on Fourier coefficients, including for spatially correlated noise that Noise2Noise cannot handle.

desk verdict The Fourier-domain noisy-supervision theorem is sound and useful; the independence claim is false but not load-bearing. read the letter →

arxiv 2506.00564 v1 pith:LNNJMTXC submitted 2025-05-31 eess.IV cs.CV

classification eess.IVcs.CV MSC 94A0860F0562E20
keywords noisysupervisionimagerestorationFourierdomainself-superviseddenoisingspatiallycorrelatednoisestriperemovalstatisticalequivalenceweaklysupervisedlearning
verification ladder T0 review T1 audit T2 compute T3 formal

The pith

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The reading

The paper tries to establish that image-restoration networks can be trained with noisy images as targets, rather than clean ones, if the loss is computed in the Fourier domain. Its central theorem states that, when the noise's Fourier coefficients are zero-mean Gaussian, the expected Fourier-domain loss with noisy targets is identical to a clean-target loss with a slightly blurred penalty, and both have the same optimum: the clean image. If this is right, practitioners can collect one noisy observation per scene and still match clean-target training, including for spatially correlated noise such as stripes and periodic patterns, where the standard Noise2Noise argument fails. The authors support the theorem with a proof that Fourier coefficients of a wide range of noise converge to independent Gaussians, and with experiments on denoising, super-resolution, and deblurring.

What carries the argument

The 2D discrete Fourier transform is the central object: its coefficients are global weighted sums of all pixels, and for spatially correlated noise they are sparse, affecting only a few frequencies. Two supporting mechanisms carry the argument: the convolution model n = h * η, whose transform variance is |F(h)|^2 var[F(η)], showing which coefficients are corrupted; and the identity ϕ = φ * p, which converts the expected noisy-target loss into a clean-target loss with a blurred penalty. The paper proves coefficient-wise Gaussian convergence using cumulants and the central limit theorem, and independence follows from orthogonality of the DFT basis.

What would settle it

Train IR-NSF on a dataset where every image patch is unique (no repeated or similar patches) and the target contains spatially correlated noise; if the restored PSNR then falls clearly below clean-target training while Noise2Noise also fails, the self-similarity replacement in Remark 7 is the broken link. A more direct check: compare the per-coefficient gradient variance under single-target and expected losses; if they differ substantially, the practical equivalence can fail even where Theorem 3.3 holds.

Watch

Extended reading notes

Core claim

Training a restoration network on noisy targets is statistically equivalent to training on clean targets, provided the loss is computed on Fourier coefficients and the target noise has zero-mean Gaussian Fourier coefficients. The key identity is E[L_φ(fθ(x), y)] = L_ϕ(fθ(x), z), where ϕ = φ * p is the penalty blurred by the noise coefficient distribution p; the minimizer of both is the clean image z. The paper also proves that Fourier coefficients of i.i.d. noise and of correlated noise n = h * η converge in distribution to independent Gaussian variables as the image grows, so the assumption covers Poisson-Gaussian noise, uniform noise, stripe noise, and periodic noise. This extends noisy supervision to spatially correlated noise, which Noise2Noise cannot handle, and lets the loss be restricted to corrupted coefficients in cases like stripe removal.

Load-bearing premise

The theorem requires averaging the loss over many noise realizations, but the implemented training uses a single noisy target per input, relying on repeated similar image patches to supply that average; there is no proof or error bound that this replacement works.

Editorial extensions

If this is right

  • A practitioner can skip the denoising step when collecting training pairs and use noisy targets directly, obtaining sharper results than pseudo-clean targets generated by BM3D.
  • Unsupervised stripe removal can be built by applying the Fourier loss only to the corrupted coefficients (k=0 for row noise), leaving image structure and pixel-wise noise intact.
  • The framework works across three restoration tasks (denoising, super-resolution, deblurring) and six network architectures, so the equivalence is not tied to a specific model.
  • When targets carry periodic or stripe noise, IR-NSF needs less training data than Noise2Noise, because the noise occupies few Fourier coefficients and averages out faster.

Reading between the lines

Editorial extensions of the paper, not claims the author makes directly.

  • If the single-target replacement in Remark 7 is a real statistical effect, it should be measurable: one could estimate the effective number of independent noise samples per Fourier coefficient and test whether the gradient noise variance matches the theorem's prediction.
  • The blurred-penalty view suggests an unexplored link to robust losses: because φ * p is a smoothed version of φ, noisy-target Fourier training may be inherently more tolerant to outliers in the target than pixel-space training.
  • The same equivalence might extend to other global transforms (wavelets, DCT, learned spectral transforms) wherever coefficients of structured noise are sparse and approximately Gaussian, offering a recipe for noisy supervision beyond the Fourier basis.
  • A testable practical claim: for scenes with unique textures and few self-similar patches, the gap between IR-NSF and clean-target training should widen, which could provide a data-collection criterion for when two noisy captures are worth collecting.
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Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, and a circularity audit.

Referee Report

3 major / 6 minor

Summary. The paper proposes IR-NSF, a framework for training image restoration networks from noisy targets by defining the training loss in the 2D-DFT domain. The central theoretical result (Theorem 3.3) states that if the target noise is zero-mean and its Fourier coefficients are Gaussian, then the expected Fourier-domain loss with noisy targets equals a blurred-penalty loss with clean targets, and the minimizer is exactly the clean image. The paper also analyzes the asymptotic distribution of Fourier coefficients for i.i.d. and spatially correlated noise, and supports the theory with extensive experiments on grayscale denoising, color super-resolution, and deblurring, including real-world SIDD and ReLoBlur datasets, as well as an unsupervised stripe removal application.

Significance. The core idea is original and timely: it extends Noise2Noise-style noisy supervision to spatially correlated noise by moving the loss to the Fourier domain, where the noise has a simpler distribution and the loss encodes global structure. As I read it, the main intended conclusion of Theorem 3.3 is correct under the stated assumptions, and the experimental validation is broad (two network architectures per task, six test sets, real-world datasets) and strongly supports the claim that Fourier-domain noisy supervision can match clean-target performance. The paper also ships public code and trained models, which is a substantial reproducibility asset. The main caveats are a false independence statement in Theorems 3.1(ii)/3.2(ii), a notational imprecision in the equivalence theorem regarding per-frequency noise variances, and an unsupported heuristic bridging the theorem to the implemented single-sample loss. These issues are fixable without changing the central result.

major comments (3)
  1. [Theorems 3.1(ii)/3.2(ii) and Appendix A] Theorems 3.1(ii) and 3.2(ii) assert that the Fourier coefficients of real-valued noise are mutually independent. This is false as stated. For a real-valued n, the 2D-DFT satisfies F(n)[U-k,V-l] = conj(F(n)[k,l]), so a(n)[U-k,V-l] = a(n)[k,l] and b(n)[U-k,V-l] = -b(n)[k,l]; such coefficients are deterministically related, not independent. The proof in Appendix A uses the orthogonality of the DFT basis to conclude that coefficients are uncorrelated, but the diagonal complex covariance E[F(n)[k,l] conj(F(n)[k',l'])] does not imply zero covariance between the real components of conjugate-symmetric pairs. The authors should correct the theorem statements (e.g., restrict independence to coefficients not linked by conjugate symmetry) and adjust the abstract/contributions, which currently claim 'independence' as a key motivation. This does not affect Theorem 3.3, whose proof only uses the marginal Gaussianity of each coefficient.
  2. [Theorem 3.3, Eq. (10), Appendix C] Equation (10) states the equivalence using a single blurred loss L_phi with one penalty phi = phi * p. However, the Fourier coefficients of noise have different variances across frequencies: for i.i.d. noise the DC coefficient has variance sigma_n^2/(UV) while other coefficients have variance sigma_n^2/(2UV) (Remark 2), and for correlated noise the variance is |F(h)|^2 times this (Eq. (8)). The correct equivalence is per-coefficient: E[L_phi(f(x),y)] = sum_{k,l} [phi_{k,l}(a(f)-a(z)) + phi_{k,l}(b(f)-b(z))] with phi_{k,l} = phi * p_{k,l}, where p_{k,l} is the zero-mean Gaussian density with the variance of that coefficient. The proof in Appendix C derives the single-component identity correctly, but the extension to a single phi in (10) does not follow. The minimizer statement (ii) remains true because each phi_{k,l} is minimized at 0, so the central conclusion is intact, but the theorem statement needs to be rewritten to use per-frequency blurring kernels.
  3. [Remark 7 and Eq. (11)] Remark 7 justifies the implemented single-sample loss in Eq. (11) by asserting that similar patches across the image and training set act as repeated samples, providing an implicit expectation over noise. This is a heuristic with no proof or error bound. The standard and correct justification is empirical risk minimization: if the training pairs are i.i.d. draws from the data distribution, then the empirical loss (11) is an unbiased estimator of the population risk, and its gradient is an unbiased estimator of the risk gradient, so SGD with one noisy target per input minimizes the expected loss of Theorem 3.3. The authors should replace the self-similarity argument with this reasoning, or provide a concrete bound; the current remark suggests a mechanism that is neither necessary nor established.
minor comments (6)
  1. [Section 4.4.1] The name 'Neighbor2Neighrbor' is a typo and should be 'Neighbor2Neighbor'.
  2. [Figure 11 caption] 'denosing' should be 'denoising'.
  3. [Section 5.2] 'CHIRS' should be 'CHRIS' (the dataset is the Compact High Resolution Imaging Spectrometer dataset).
  4. [Figure 12 caption] 'T arget' contains an unwanted space and should read 'Target'.
  5. [Appendix A] In the proof of Theorem 3.1(i), the condition 'kl̸=0' should be phrased as 'except k=l=0', since the same argument applies to k=0,l≠0 and to k≠0,l=0.
  6. [Section 4.1] The experiments use a Huber loss for denoising, but the Huber parameter is never specified; please provide the numerical value for reproducibility.

Circularity Check

0 steps flagged · score 0.0 of 10

No significant circularity: Theorem 3.3 is derived from explicit zero-mean Gaussian Fourier-coefficient assumptions and a monotonicity condition on the penalty, with no fitted parameter or self-citation chain carrying the result.

full rationale

I examined the claimed derivation chain. The central result (Theorem 3.3, Eq. (10)) is a direct consequence of the stated assumptions: if each Fourier coefficient of the noise has density p(t) and is independent of the input, then E[phi(a_f - a_y)] = phi * p (a_f - a_z) by the convolution identity, and the Appendix C derivative argument proves that phi * p has its global minimum at zero when phi increases with |t| and p is zero-mean Gaussian. Thus no predicted value is secretly a fitted value, and no parameter is calibrated to the clean image. Theorems 3.1 and 3.2 are CLT-style supporting analysis; although the pairwise-independence assertion in Theorems 3.1(ii) and 3.2(ii) is overstated because real-valued 2D-DFT coefficients obey Hermitian symmetry, that flaw is a correctness issue, not a circular reduction, and Theorem 3.3 does not use independence across coefficients. The practical loss in Eq. (11) (Section 3.3, Remark 7) replaces the expectation in Eq. (10) with a single noisy target per input; Remark 7 justifies this only heuristically, but that is an approximation gap, not a circular definition. Self-citations (e.g., [31] for DCT coefficient analysis) serve as background analogies and do not carry the equivalence. Comparison against external benchmarks (DIV2K, SIDD, ReLoBlur) makes the experimental claims independently checkable. Overall, the derivation is self-contained under its explicit assumptions, so the circularity score is 0.

Assumptions & free parameters 2 free parameters · 6 assumptions · 0 invented entities

The central theorem is self-contained once the Gaussian-coefficient assumption is granted. The main unpaid inputs are the convolution noise model for correlated noise, the finite-image Gaussian approximation, and the self-similarity heuristic that turns a theoretical expectation into a single-sample loss. No fitted constants are used in the derivation; the loss penalty and USR amplification factor are hand-selected.

free parameters (2)
  • Loss penalty φ(t) and Huber parameter = Huber for denoising; L1 (q=1) for super-resolution and deblurring; Huber δ not reported
    Theorem 3.3 holds for any even increasing φ, so the specific choice is not fitted to make the derivation work, but it is hand-selected and affects the reported metrics.
  • USR noise amplification factor ε = not reported (stated as ε>1)
    Introduced in Section 5.2 to compensate under-estimated stripe noise in the unsupervised stripe removal; its value is not given and affects USR results.
assumptions (6)
  • standard math Central limit theorem / Lyapunov conditions for weighted sums of i.i.d. noise with bounded cumulants
    Used in Theorem 3.1 to show Fourier coefficients of i.i.d. noise converge to Gaussian.
  • domain assumption Correlated noise is modeled as n = h * η with zero-mean i.i.d. η
    Theorem 3.2 relies on this model from [25],[26]; not all spatially correlated noise, e.g. non-stationary noise, fits it.
  • domain assumption Finite-image Fourier coefficients are approximately Gaussian and independent
    Theorems 3.1 and 3.2 are asymptotic in UV; the practical loss (9)-(12) treats the approximation as exact for images around 480x480.
  • domain assumption Target noise is zero-mean and independent of the input
    Assumed in Theorem 3.3 and satisfied by two independent captures of the same scene; may fail for signal-dependent or input-correlated noise.
  • ad hoc to paper Self-similar patches make the single-sample loss (11) approximate the expectation in (10)
    Remark 7 gives this heuristic without proof; it is load-bearing for the implemented training procedure.
  • domain assumption The correlation kernel h has sparse |F(h)| for diverse correlated noise
    Section 3.2.2 cites [26] for sparsity; used to explain the advantage over N2N and to restrict the USR loss to k=0.

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Pith. "Pith review of Image Restoration Learning via Noisy Supervision in the Fourier Domain." pith.science (2026). https://pith.science/paper/LNNJMTXC

@misc{pith2026250600564,
  author       = {Pith},
  title        = {Pith review of: Image Restoration Learning via Noisy Supervision in the Fourier Domain},
  year         = {2026},
  howpublished = {\url{https://pith.science/paper/LNNJMTXC}},
  note         = {Machine review of arXiv:2506.00564}
}
read the original abstract

Noisy supervision refers to supervising image restoration learning with noisy targets. It can alleviate the data collection burden and enhance the practical applicability of deep learning techniques. However, existing methods suffer from two key drawbacks. Firstly, they are ineffective in handling spatially correlated noise commonly observed in practical applications such as low-light imaging and remote sensing. Secondly, they rely on pixel-wise loss functions that only provide limited supervision information. This work addresses these challenges by leveraging the Fourier domain. We highlight that the Fourier coefficients of spatially correlated noise exhibit sparsity and independence, making them easier to handle. Additionally, Fourier coefficients contain global information, enabling more significant supervision. Motivated by these insights, we propose to establish noisy supervision in the Fourier domain. We first prove that Fourier coefficients of a wide range of noise converge in distribution to the Gaussian distribution. Exploiting this statistical property, we establish the equivalence between using noisy targets and clean targets in the Fourier domain. This leads to a unified learning framework applicable to various image restoration tasks, diverse network architectures, and different noise models. Extensive experiments validate the outstanding performance of this framework in terms of both quantitative indices and perceptual quality.

Figures

Figures reproduced from arXiv: 2506.00564 by the authors.

Figure 2
Figure 2. Histograms of noise in the spatial domain and its coefficient in [PITH_FULL_IMAGE:figures/full_fig_p004_2.png] view at source ↗
Figure 4
Figure 4. Statistical equivalence. Utilizing φ(t) with noisy targets is statis￾tically equivalent to utilizing ϕ(t) = φ(t) ∗ p(t) with clean targets. The p(t) corresponds to the zero-mean Gaussian distribution with σ = 0.2. maintain both the independence and the sparsity in the Fourier domain. These findings emphasize the advantages of utilizing the Fourier domain for noisy supervision and provide insights into the developmen… view at source ↗
Figure 5
Figure 5. Illustration of training pairs for DN, SR, and DB. These images [PITH_FULL_IMAGE:figures/full_fig_p006_5.png] view at source ↗
Figures from the paper (10 more)
Figure 6
Figure 6. Figure 6: (b), the convergence curves for IR-NSF and IR-CSF are almost consistent everywhere. As for the DN experiment shown in [PITH_FULL_IMAGE:figures/full_fig_p007_6.png]
Figure 7
Figure 7. Figure 7: Visual results of denoising experiments. The image contrast is adjusted for better comparison. [PITH_FULL_IMAGE:figures/full_fig_p008_7.png]
Figure 8
Figure 8. Figure 8: Visual results of super-resolution experiments. [PITH_FULL_IMAGE:figures/full_fig_p009_8.png]
Figure 9
Figure 9. Figure 9: Visual results of deblurring experiments. [PITH_FULL_IMAGE:figures/full_fig_p009_9.png]
Figure 10
Figure 10. Figure 10: Visual results of deblurring experiments on ReLoBlur. The [PITH_FULL_IMAGE:figures/full_fig_p010_10.png]
Figure 11
Figure 11. Figure 11: Illustration of the data collection pipeline adopted by existing [PITH_FULL_IMAGE:figures/full_fig_p011_11.png]
Figure 14
Figure 14. Figure 14: PSNR (dB) on Urban100 as a function of training step. For (a), the noise type is the Poisson-Gaussian noise and the training set is the DIV2K. For (b), the noise type is the mixture of Poisson-Gaussian and periodic noise. The training set is the combination of DIV2K a…
Figure 15
Figure 15. Figure 15: Visual results of denoising experiments under limited train [PITH_FULL_IMAGE:figures/full_fig_p011_15.png]
Figure 16
Figure 16. Figure 16: Visual comparison among VSNR [25], SEID [42], and USR. [PITH_FULL_IMAGE:figures/full_fig_p012_16.png]
Figure 17
Figure 17. Figure 17: Visual results on real-world remote sensing dataset CHRIS. [PITH_FULL_IMAGE:figures/full_fig_p013_17.png]

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Pith tools

Reviewed August 7, 2026 · model on record in the stance chip above.