Photometric Stereo
Photometric Stereo
Standard reconstruction benchmark — forward model perfectly known, no calibration needed. Score = 0.5 × clip((PSNR−15)/30, 0, 1) + 0.5 × SSIM
| # | Method | Score | PSNR (dB) | SSIM | Source | |
|---|---|---|---|---|---|---|
| 🥇 |
PS-Transformer
PS-Transformer Ikehata, ICCV 2023
34.2 dB
SSIM 0.945
Checkpoint unavailable
|
0.792 | 34.2 | 0.945 | ✓ Certified | Ikehata, ICCV 2023 |
| 🥈 |
CNN-PS
CNN-PS Ikehata, ECCV 2018
32.5 dB
SSIM 0.915
Checkpoint unavailable
|
0.749 | 32.5 | 0.915 | ✓ Certified | Ikehata, ECCV 2018 |
| 🥉 | Robust PCA | 0.635 | 28.5 | 0.820 | ✓ Certified | Wu et al., ECCV 2010 |
| 4 | LS Normal Est. | 0.517 | 25.0 | 0.700 | ✓ Certified | Woodham, Opt. Eng. 1980 |
Dataset: PWM Benchmark (4 algorithms)
Blind Reconstruction Challenge — forward model has unknown mismatch, must calibrate from data. Score = 0.4 × PSNR_norm + 0.4 × SSIM + 0.2 × (1 − ‖y − Ĥx̂‖/‖y‖)
| # | Method | Overall Score | Public PSNR / SSIM |
Dev PSNR / SSIM |
Hidden PSNR / SSIM |
Trust | Source |
|---|---|---|---|---|---|---|---|
| 🥇 | PS-Transformer + gradient | 0.715 |
0.795
32.82 dB / 0.951
|
0.707
28.93 dB / 0.899
|
0.643
24.98 dB / 0.802
|
✓ Certified | Ikehata, ICCV 2023 |
| 🥈 | CNN-PS + gradient | 0.683 |
0.771
31.04 dB / 0.931
|
0.647
25.72 dB / 0.824
|
0.631
24.83 dB / 0.797
|
✓ Certified | Ikehata, ECCV 2018 |
| 🥉 | Robust PCA + gradient | 0.643 |
0.679
26.58 dB / 0.848
|
0.647
24.93 dB / 0.800
|
0.604
24.11 dB / 0.772
|
✓ Certified | Wu et al., ECCV 2010 |
| 4 | LS Normal Est. + gradient | 0.548 |
0.591
22.73 dB / 0.720
|
0.537
20.75 dB / 0.634
|
0.516
20.49 dB / 0.622
|
✓ Certified | Woodham, Opt. Eng. 1980 |
Complete score requires all 3 tiers (Public + Dev + Hidden).
Join the competition →Full-access development tier with all data visible.
What you get & how to use
What you get: Measurements (y), ideal forward operator (H), spec ranges, ground truth (x_true), and true mismatch spec.
How to use: Load HDF5 → compare reconstruction vs x_true → check consistency → iterate.
What to submit: Reconstructed signals (x_hat) and corrected spec as HDF5.
Public Leaderboard
| # | Method | Score | PSNR | SSIM |
|---|---|---|---|---|
| 1 | PS-Transformer + gradient | 0.795 | 32.82 | 0.951 |
| 2 | CNN-PS + gradient | 0.771 | 31.04 | 0.931 |
| 3 | Robust PCA + gradient | 0.679 | 26.58 | 0.848 |
| 4 | LS Normal Est. + gradient | 0.591 | 22.73 | 0.72 |
Spec Ranges (4 parameters)
| Parameter | Min | Max | Unit |
|---|---|---|---|
| light_direction_error | -1.0 | 2.0 | degpersource |
| light_intensity_calibration | 0.96 | 1.08 | - |
| non_lambertian_surface_fraction | -6.0 | 12.0 | - |
| cast_shadow_fraction | -3.0 | 6.0 | ofpixels |
Blind evaluation tier — no ground truth available.
What you get & how to use
What you get: Measurements (y), ideal forward operator (H), and spec ranges only.
How to use: Apply your pipeline from the Public tier. Use consistency as self-check.
What to submit: Reconstructed signals and corrected spec. Scored server-side.
Dev Leaderboard
| # | Method | Score | PSNR | SSIM |
|---|---|---|---|---|
| 1 | PS-Transformer + gradient | 0.707 | 28.93 | 0.899 |
| 2 | CNN-PS + gradient | 0.647 | 25.72 | 0.824 |
| 3 | Robust PCA + gradient | 0.647 | 24.93 | 0.8 |
| 4 | LS Normal Est. + gradient | 0.537 | 20.75 | 0.634 |
Spec Ranges (4 parameters)
| Parameter | Min | Max | Unit |
|---|---|---|---|
| light_direction_error | -1.2 | 1.8 | degpersource |
| light_intensity_calibration | 0.952 | 1.072 | - |
| non_lambertian_surface_fraction | -7.2 | 10.8 | - |
| cast_shadow_fraction | -3.6 | 5.4 | ofpixels |
Fully blind server-side evaluation — no data download.
What you get & how to use
What you get: No data downloadable. Algorithm runs server-side on hidden measurements.
How to use: Package algorithm as Docker container / Python script. Submit via link.
What to submit: Containerized algorithm accepting y + H, outputting x_hat + corrected spec.
Hidden Leaderboard
| # | Method | Score | PSNR | SSIM |
|---|---|---|---|---|
| 1 | PS-Transformer + gradient | 0.643 | 24.98 | 0.802 |
| 2 | CNN-PS + gradient | 0.631 | 24.83 | 0.797 |
| 3 | Robust PCA + gradient | 0.604 | 24.11 | 0.772 |
| 4 | LS Normal Est. + gradient | 0.516 | 20.49 | 0.622 |
Spec Ranges (4 parameters)
| Parameter | Min | Max | Unit |
|---|---|---|---|
| light_direction_error | -0.7 | 2.3 | degpersource |
| light_intensity_calibration | 0.972 | 1.092 | - |
| non_lambertian_surface_fraction | -4.2 | 13.8 | - |
| cast_shadow_fraction | -2.1 | 6.9 | ofpixels |
Blind Reconstruction Challenge
ChallengeGiven measurements with unknown mismatch and spec ranges (not exact params), reconstruct the original signal. A method must be evaluated on all three tiers for a complete score. Scored on a composite metric: 0.4 × PSNR_norm + 0.4 × SSIM + 0.2 × (1 − ‖y − Ĥx̂‖/‖y‖).
Measurements y, ideal forward model H, spec ranges
Reconstructed signal x̂
Spec DAG — Forward Model Pipeline
M → C → D
Mismatch Parameters
| Symbol | Parameter | Description | Nominal | Perturbed |
|---|---|---|---|---|
| l_d | light_direction_error | Light direction error (deg per source) | 0.0 | 1.0 |
| l_i | light_intensity_calibration | Light intensity calibration (-) | 1.0 | 1.04 |
| n_s | non_lambertian_surface_fraction | Non-Lambertian surface fraction (-) | 0.0 | 6.0 |
| c_s | cast_shadow_fraction | Cast shadow fraction (of pixels) | 0.0 | 3.0 |
Credits System
Spec Primitives Reference (11 primitives)
Free-space or medium propagation kernel (Fresnel, Rayleigh-Sommerfeld).
Spatial or spatio-temporal amplitude modulation (coded aperture, SLM pattern).
Geometric projection operator (Radon transform, fan-beam, cone-beam).
Sampling in the Fourier / k-space domain (MRI, ptychography).
Shift-invariant convolution with a point-spread function (PSF).
Summation along a physical dimension (spectral, temporal, angular).
Sensor readout with gain g and noise model η (Gaussian, Poisson, mixed).
Patterned illumination (block, Hadamard, random) applied to the scene.
Spectral dispersion element (prism, grating) with shift α and aperture a.
Sample or gantry rotation (CT, electron tomography).
Spectral filter or monochromator selecting a wavelength band.