Skip to content

This repository is the official data source for the paper "Advancing blind hyperspectral unmixing in remote sensing: comparing deep-inspired subspace learning methods" by G. Settembre, F. Esposito, N. Del Buono

License

Notifications You must be signed in to change notification settings

gaetanosettembre/data_unmixing

Folders and files

NameName
Last commit message
Last commit date

Latest commit

 

History

10 Commits
 
 
 
 
 
 
 
 
 
 

Repository files navigation

Datasets & Ground Truths for

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).


At a glance

  • 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 .fig metadata files.

Repository structure

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

Dataset cards

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.

Cuprite (benchmark)

  • 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")

Samson (benchmark)

  • Dims: 95 × 95 × 156 (H × W × B)
  • Materials (K): 3 ("#1 Soil", "#2 Tree" and "#3 Water")

Urban 4 (benchmark)

  • Dims: 307 × 307 × 162
  • Materials (K): 4 ("#1 Asphalt", "#2 Grass", "#3 Tree" and "#4 Roof")

Urban 5 (benchmark)

  • Dims: 307 × 307 × 162
  • Materials (K): 5 ("#1 Asphalt", "#2 Grass", "#3 Tree", "#4 Roof" and "#5 Dirt")

Urban 6 (benchmark)

  • Dims: 307 × 307 × 162
  • Materials (K): 6 ("#1 Asphalt", "#2 Grass", "#3 Tree", "#4 Roof", "#5 Metal", and "6 Dirt")

Jasper Ridge (benchmark)

  • Dims: 100 × 100 × 198
  • Materials (K): 4 ("#1 Road", "#2 Soil", "#3 Water" and "#4 Tree")

PRISMA – Alimini (real scene)

  • 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.

PRISMA – Limassol Fire (real scene)

  • 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.


File formats & conventions

  • Cubes: H × W × B
    • .mat (MATLAB) with variable name Y.
  • Endmembers ground truth: K × B matrix (materials × bands).
  • Abundances ground truth: K × H × W tensor (materials × height × width).

Licensing & usage

  • 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.


How to cite

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 
}

Acknowledgements

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.


Contact

For questions about the data or PRISMA access, please contact:
Gaetano Settembre[email protected]

About

This repository is the official data source for the paper "Advancing blind hyperspectral unmixing in remote sensing: comparing deep-inspired subspace learning methods" by G. Settembre, F. Esposito, N. Del Buono

Topics

Resources

License

Stars

Watchers

Forks

Releases

No releases published

Packages

No packages published