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Paper · 2303.15724 · CVPR · 2023

Scalable, Detailed and Mask-Free Universal Photometric Stereo

Satoshi Ikehata

arXiv · PDF · Open in the Atlas

Code that ran

We lifted 8 functions out of this paper's own repositories and ran 1 of them in a sandbox. "Ran" means the function executed on a synthesized input and returned a value. It is not a reproduction of the paper's results.

RepositoryRoleRan
satoshi-ikehata/sdm-unips-cvpr2023 — 1 of 8
FunctionStatusWhere it lives
PredictionHead Ran satoshi-ikehata/sdm-unips-cvpr2023/sdm_unips/modules/model/model.py
pointer only (licence: NOASSERTION) · get_code("18c46000813125d3")
GLC_Aggregation Not yet run satoshi-ikehata/sdm-unips-cvpr2023/sdm_unips/modules/model/model.py
pointer only (licence: NOASSERTION) · get_code("ab46129d2b2f846c")
GLC_Upsample Not yet run satoshi-ikehata/sdm-unips-cvpr2023/sdm_unips/modules/model/model.py
pointer only (licence: NOASSERTION) · get_code("3d7b3b540b5e04c2")
ImageFeatureExtractor Not yet run satoshi-ikehata/sdm-unips-cvpr2023/sdm_unips/modules/model/model.py
pointer only (licence: NOASSERTION) · get_code("29ae70b405dc9e43")
ImageFeatureFusion Not yet run satoshi-ikehata/sdm-unips-cvpr2023/sdm_unips/modules/model/model.py
pointer only (licence: NOASSERTION) · get_code("45a21fe9e5c6bcb2")
Net Not yet run satoshi-ikehata/sdm-unips-cvpr2023/sdm_unips/modules/model/model.py
pointer only (licence: NOASSERTION) · get_code("98f86a99159bc9cb")
Regressor Not yet run satoshi-ikehata/sdm-unips-cvpr2023/sdm_unips/modules/model/model.py
pointer only (licence: NOASSERTION) · get_code("215a8657c68da22c")
ScaleInvariantSpatialLightImageEncoder Not yet run satoshi-ikehata/sdm-unips-cvpr2023/sdm_unips/modules/model/model.py
pointer only (licence: NOASSERTION) · get_code("13ca5597f1641766")

Repositories linked to this paper

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Abstract

Surface normal map SDM-UniPS (Ours) Input image (1st out of 9) UniPS [Ikehata2022] 3D Scanner (EinScan-SE) INPUT: Multiple images under varying unknown lighting conditions 1st 2nd 23rd Figure 1. Given multiple images under unknown spatially-varying illuminations, our method can recover the detailed surface normal map of non-convex, non-Lambertian surfaces (Left). Our method even surpasses the level of detail provided by consumer 3-D scanners (Right).

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have("2303.15724")

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