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--- |
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license: cc-by-4.0 |
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task_categories: |
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- robotics |
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- feature-extraction |
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language: |
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- en |
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tags: |
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- Space |
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- Structure-from-Motion |
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- SfM |
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- SLAM |
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- Asteroid |
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- Stereophotoclinometry |
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pretty_name: Photoclinometry-from-Motion (PhoMo) |
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size_categories: |
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- n<1K |
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configs: |
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- config_name: default |
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data_files: |
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- split: train |
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path: data/train-* |
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dataset_info: |
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features: |
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- name: image |
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dtype: image |
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- name: site |
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dtype: string |
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- name: body |
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dtype: string |
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- name: fits_path |
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dtype: string |
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- name: npy_path |
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dtype: string |
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- name: id |
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dtype: string |
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splits: |
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- name: train |
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num_bytes: 92236737 |
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num_examples: 99 |
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download_size: 92237643 |
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dataset_size: 92236737 |
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--- |
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<div align="center"> |
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<img src="assets/phomo.png" alt="logo" width="400"> |
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<h1>Photoclinometry-from-Motion (PhoMo)</h1> |
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<a href="https://huggingface.co/datasets/travisdriver/phomo-data"><img src="https://img.shields.io/badge/🤗-Hugging%20Face-yellow.svg" alt="HuggingFace"></a> |
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<a href="https://arxiv.org/abs/2504.08252"><img src="https://img.shields.io/badge/arXiv-2504.08252-b31b1b" alt="arXiv"></a> |
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[Travis Driver](https://travisdriver.github.io/), [Andrew Vaughan](https://www.linkedin.com/in/andrewtvaughan/), [Yang Cheng](https://www-robotics.jpl.nasa.gov/who-we-are/people/yang_cheng/), [Adnan Ansar](https://www-robotics.jpl.nasa.gov/who-we-are/people/adnan_ansar/), [John Christian](https://ae.gatech.edu/directory/person/john-christian), [Panagiotis Tsiotras](https://ae.gatech.edu/directory/person/panagiotis-tsiotras) |
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</div> |
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#### This is the official repository for [Stereophotoclinometry Revisited](https://arxiv.org/abs/2504.08252), which is currently under review for publication to AIAA's [Journal of Guidance, Control, and Dynamics (JGCD)](https://arc.aiaa.org/loi/jgcd) |
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**Photoclinometry-from-Motion (PhoMo)** is a framework for _autonomous_ image-based surface reconstruction and characterization of small celestial bodies. PhoMo integrates photoclinometry into a structure-from-motion (SfM) pipeline that leverages deep learning-based keypoint extraction and matching (i.e., [RoMa](https://github.com/Parskatt/RoMa)) to enable _simultaneous_ optimization of the spacecraft pose, landmark positions, Sun vectors, and surface normals and albedos. |
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If you find our datasets or results useful for your research, please use the following citation: |
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```bibtex |
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@article{driver2025phomo, |
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title={Stereophotoclinometry Revisited}, |
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author={Driver, Travis and Vaughan, Andrew and Cheng, Yang, and Ansar, Adnan and Christian, John and Tsiotras, Panagiotis}, |
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journal={arXiv:2504.08252}, |
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year={2025}, |
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pages={1--45} |
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} |
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``` |
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<!--- |
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## Dataset Structure |
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Each directory contains a subdirectory for each of the sites used in the paper, i.e., Cornelia (`cornelia/`), Ahuna Mons (`ahunamons/`), and Ikapati (`ikapati/`). |
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`images/`: Contains the input images for each site (i.e., Cornelia, Ahuna Mons, and Ikapati) in multiple formats. |
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- `*_calib.npy`: Radiometrically calibrated to units of reflectance (L/F). |
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- `*_uncalib.npy`: |
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- `*.png`: |
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---> |
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