Advancing blind hyperspectral unmixing in remote sensing: comparing deep-inspired subspace learning methods
This repository hosts the datasets, ground truths, and metadata used in the manuscript above.
No training or evaluation code is included — the repo focuses solely on data distribution.
If you use these data, please cite the paper (see How to cite).
- Scope: benchmark cubes and real-scene metadata/annotations for hyperspectral unmixing (HU).
- Included: data cubes, endmember spectra, abundance maps.
- Excluded: model implementations, training scripts, evaluation pipelines.
- Format:
.mat, plus.figmetadata files.
Datasets/
Cuprite/
- Cuprite_GT_nEnd12.mat
- Cuprite_data_R188.mat
Jasper/
- jasperRidge2_R198.mat
- Jasper_GT.mat
- end4_Materials.fig
- end4_Abundance.fig
Samson/
- Samson.mat
- Samson_GT.mat
- end3_Abundances.fig
- end3_Materials.fig
Urban/
- Urban.mat
- end4_groundTruth.mat
- end5_groundTruth.mat
- end6_groundTruth.mat
- Figures of endmembers and abundance maps
README.md
Below we summarize typical configurations used in HU literature. Exact shapes may differ slightly depending on band-selection and pre-processing; the per-folder README.md specifies what is provided here.
- Dims:
250 × 191 × 188(H × W × B) - Materials (K): 12 ("#1 Alunite", "#2 Andradite", "#3 Buddingtonite", "#4 Dumortierite", "#5 Kaolinite1", "#6 Kaolinite2", "#7 Muscovite", "#8 Montmorillonite", "#9 Nontronite", "#10 Pyrope", "#11 Sphene", "#12 Chalcedony")
- Dims:
95 × 95 × 156(H × W × B) - Materials (K): 3 ("#1 Soil", "#2 Tree" and "#3 Water")
- Dims:
307 × 307 × 162 - Materials (K): 4 ("#1 Asphalt", "#2 Grass", "#3 Tree" and "#4 Roof")
- Dims:
307 × 307 × 162 - Materials (K): 5 ("#1 Asphalt", "#2 Grass", "#3 Tree", "#4 Roof" and "#5 Dirt")
- Dims:
307 × 307 × 162 - Materials (K): 6 ("#1 Asphalt", "#2 Grass", "#3 Tree", "#4 Roof", "#5 Metal", and "6 Dirt")
- Dims:
100 × 100 × 198 - Materials (K): 4 ("#1 Road", "#2 Soil", "#3 Water" and "#4 Tree")
- Dims: typically large swaths (subsetted to
1000 × 1000, ~230 valid bands after removal) - Materials (K): 4 ("#1 Water", "#2 Soil", "#3 Clouds", "#4 Vegetation")
Redistribution notice: raw PRISMA imagery is not included here.
- Dims: similar to Alimini (subsetted), ~230 valid bands after removal
- Materials (K): 4 ("#1 Water", "#2 Clouds", "#3 Vegetation", "#4 Burned area")
Redistribution notice: raw PRISMA imagery is not included here.
- Cubes:
H × W × B.mat(MATLAB) with variable nameY.
- Endmembers ground truth:
K × Bmatrix (materials × bands). - Abundances ground truth:
K × H × Wtensor (materials × height × width).
- Benchmark data (Cuprite, Samson, Urban, Jasper Ridge) are provided for research and educational use; please respect the original dataset terms where applicable.
- PRISMA imagery is not redistributed here due to licensing; this repo includes only derived metadata and expert-derived reference endmembers. For access to raw imagery, please contact the corresponding author listed in the manuscript or the data provider.
A repository-level LICENSE file is included. If you need a different license, please open an issue.
If this repository or the provided ground truths/metadata are useful to your work, please cite:
Gaetano Settembre, Flavia Esposito, Nicoletta Del Buono.
Advancing blind hyperspectral unmixing in remote sensing: comparing deep-inspired subspace learning methods. Manuscript. Advanced Modeling and Simulation in Engineering Sciences 12, 30 (2025). https://doi.org/10.1186/s40323-025-00313-6.
@article{Settembre2025,
title = {Advancing blind hyperspectral unmixing in remote sensing: comparing deep-inspired subspace learning methods},
volume = {12},
ISSN = {2213-7467},
url = {http://dx.doi.org/10.1186/s40323-025-00313-6},
DOI = {10.1186/s40323-025-00313-6},
number = {1},
journal = {Advanced Modeling and Simulation in Engineering Sciences},
publisher = {Springer Science and Business Media LLC},
author = {Settembre, Gaetano and Esposito, Flavia and Del Buono, Nicoletta},
year = {2025},
month = oct
}We acknowledge the providers of benchmark datasets widely used in HU research and PRISMA data courtesy of the Italian Space Agency (ASI) and Planetek Italia S.r.l. We also thank all collaborators acknowledged in the manuscript.
For questions about the data or PRISMA access, please contact:
Gaetano Settembre — [email protected]