**W1**:
We thank the reviewer for the feedback. In response, we highlight two examples from our benchmarks, DAPS and PnP-DM, that illustrate the nuances of performance differences between natural image restoration tasks and the scientific inverse problems.
Both DAPS and PnP-DM achieve near state-of-the-art results on natural image restoration tasks such as inpainting and super-resolution. However, their performance significantly deteriorates in problems like Full Waveform Inversion (FWI) in InverseBench. This issue stems from their inability to account for the stability conditions required to query the forward model. For example, the numerical PDE solvers used in FWI and the Navier-Stokes equations impose strict stability constraints, such as the Courant–Friedrichs–Lewy (CFL) condition. The Langevin Monte Carlo (LMC) subroutine used by DAPS and PnP-DM introduces noisy perturbations in the input. While such noise is tolerable in natural image restoration tasks, it violates the stability conditions in these scientific inverse problems, resulting in numerical instability and unreliable gradient estimates. We discuss this in detail in lines 435–451 of the paper, where we also provide examples of these instabilities.
**Q1**:
Thank you for pointing this out; your understanding is correct. We employ a separate model, initialized with different random seeds, trained on a dataset of 50,000 non-publicly available images. This model is used to unconditionally generate 5 images for the validation dataset and 100 images for the test dataset. These generated datasets are utilized for hyperparameter tuning and evaluation.
**Q2**:
We certainly agree that investigating robustness is very important. As alluded to by your question, there are two main types of robustness that are important to study: prior mismatch and forward model G mismatch. We have added a discussion with some of our preliminary results on this research direction in Appendix B.
**Q3**:
This is a good question. We have experimented with FFHQ and ImageNet pretrained priors on black hole imaging and inverse scattering tasks. Our findings are summarized as follows: the more ill-posed a problem is, the more critical the role of the prior becomes.
Because black hole imaging is highly ill-posed, combining the FFHQ pretrained prior with PnP diffusion methods produces an image resembling a human face while still satisfying the observational black hole data with a $\chi^2$ value between 1.1 and 1.5. However, these images significantly diverge from the true black hole images, with a substantial PSNR drop of about 5–8 dB compared to in-distribution data priors. However, for the less ill-posed inverse scattering task, comparable results can be achieved between the baseline and the PnP diffusion with in-distribution priors. The table below presents the evaluation results for inverse scattering on 100 test samples. We can observe that both the FFHQ and ImageNet priors improve the results compared to the baseline, which uses only total variation (TV) as the prior.
| Methods/inverse scattering receivers | 360 | 180 | 60 |
| ------------------------------------ | ------ | ------ | ------ |
| DAPS + In-distribution Data Prior | 34.641 | 33.160 | 25.875 |
| DAPS + FFHQ Prior | 33.048 | 30.821 | 21.413 |
| DAPS + ImageNet Prior | 32.873 | 30.412 | 21.223 |
| FISTA+TV | 32.126 | 26.523 | 20.938 |
An important implementation detail to highlight is the mismatch between the dimensions of the priors and the dimensions of the tasks. For example, the typical dimension of an ImageNet pretrained prior is (3, 256, 256), while the dimension for inverse scattering is (1, 128, 128). To resolve this mismatch, we introduced a wrapper before the forward function of each task to map the prior dimensions to the task dimensions. Specifically, we downsampled the images and converted them to grayscale, aligning the (3, 256, 256) prior dimensions with the (1, 128, 128) task dimensions used in inverse scattering.