Add metadata (license, pipeline tag) and usage examples
#1
by
nielsr
HF Staff
- opened
README.md
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# π SpecCLIP: Aligning and Translating Spectroscopic Measurements for Stars
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[](https://arxiv.org/abs/2507.01939)
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**SpecCLIP** is a contrastive + domain-preserving foundation model designed to align **LAMOST LRS** spectra with **Gaia XP** spectrophotometric data.
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It learns a **general-purpose spectral embedding (768-dim)** that supports:
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For full documentation, installation instructions, examples, and end-to-end usage, please visit the **GitHub repository**:
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π [https://github.com/Xiaosheng-Zhao/SpecCLIP](https://github.com/Xiaosheng-Zhao/SpecCLIP)
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SpecCLIP consists of:
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It produces **shared embeddings** enabling multi-survey astrophysical analysis.
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---
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## π Full Documentation
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To keep the Hugging Face card concise, **all detailed instructions**, including:
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are available at the GitHub repo:
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month = jul,
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eid = {arXiv:2507.01939},
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pages = {arXiv:2507.01939},
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doi = {10.48550/arXiv.
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archivePrefix = {arXiv},
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eprint = {2507.01939},
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primaryClass = {astro-ph.IM},
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## π¬ Contact
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---
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license: mit
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pipeline_tag: feature-extraction
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---
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# π SpecCLIP: Aligning and Translating Spectroscopic Measurements for Stars
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[](https://arxiv.org/abs/2507.01939)
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**SpecCLIP** is a contrastive + domain-preserving foundation model designed to align **LAMOST LRS** spectra with **Gaia XP** spectrophotometric data.
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It learns a **general-purpose spectral embedding (768-dim)** that supports:
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* **Stellar parameter estimation**
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* **Cross-survey spectral translation** (LAMOST LRS β· Gaia XP)
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* **Similarity retrieval** across LAMOST LRS and GAIA XP spectra
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For full documentation, installation instructions, examples, and end-to-end usage, please visit the **GitHub repository**:
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π [https://github.com/Xiaosheng-Zhao/SpecCLIP](https://github.com/Xiaosheng-Zhao/SpecCLIP)
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SpecCLIP consists of:
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* **Two masked transformer encoders**
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β LAMOST LRS
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β Gaia XP
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* **Contrastive alignment loss (CLIP-style)**
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* **Domain-preserving prediction & reconstruction heads**
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* **Cross-modal decoder** for spectrum translation
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It produces **shared embeddings** enabling multi-survey astrophysical analysis.
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---
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## Sample Usage
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The following examples are adapted from the [official GitHub repository](https://github.com/Xiaosheng-Zhao/SpecCLIP).
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### Installation
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First, create a conda environment and install requirements:
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```bash
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conda create -n specclip-ai python=3.10
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conda activate specclip-ai
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conda install pytorch==2.5.1 torchvision==0.20.1 pytorch-cuda=11.8 -c pytorch -c nvidia
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conda install numpy==2.0.1 scipy==1.15.3 pandas==2.3.3 mkl mkl-service -c defaults
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pip install -r requirements.txt
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pip install -e .
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```
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### Spectral Translation
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Predict Gaia XP spectrum from LAMOST LRS:
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```python
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import json
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from spectral_retrieval import SpectralRetriever
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from predict_lrs_wclip_v0 import load_spectrum_data
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# Configuration
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with open('config_retrieval.json', 'r') as f:
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config = json.load(f)
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retriever = SpectralRetriever(**config)
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# Load the external spectra data
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wavelength, flux = load_spectrum_data('./test_data/lrs/sample1_matrix.fits')
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# Predict corresponding Gaia XP spectrum
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prediction_external = retriever.predict_cross_modal(
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query_spectrum=(wavelength, flux),
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query_type='lamost_spectra'
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)
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# Plot
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retriever.plot_cross_modal_prediction(
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prediction_external,
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save_path='./plots/external_lamost_to_gaia_prediction.png'
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)
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```
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### Spectral Similarity Search
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Find the top-4 most similar stars from Gaia XP catalog:
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```python
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# Download test data only
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!python download_and_setup.py --test-data-only
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# Build embedding database from test data
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retriever.build_embedding_database(batch_size=1000, save_path='./test_embeddings.npz')
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# Load external LAMOST spectrum
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wavelength, flux = load_spectrum_data('./test_data/lrs/sample1_matrix.fits')
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# Find similar Gaia XP spectra
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results_external_cross = retriever.find_similar_spectra(
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query_spectrum=(wavelength, flux),
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query_type='lamost_spectra',
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search_type='cross_modal',
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top_k=4
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)
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# Plot
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retriever.plot_retrieval_results(
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results_external_cross,
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save_path='./plots/external_lamost_to_gaia_cross.png'
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)
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```
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### Parameter Prediction
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**Coming soon.**
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This section will include examples of using SpecCLIP embeddings with downstream models (e.g., MLP, SBI) for stellar-parameter prediction.
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---
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## π Full Documentation
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To keep the Hugging Face card concise, **all detailed instructions**, including:
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* Installation
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* Parameter prediction
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* Spectral translation
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* Retrieval
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* Full examples (Python + figures)
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* Acknowledgments
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are available at the GitHub repo:
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month = jul,
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eid = {arXiv:2507.01939},
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pages = {arXiv:2507.01939},
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doi = {10.48550/arXiv.250701939},
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archivePrefix = {arXiv},
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eprint = {2507.01939},
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primaryClass = {astro-ph.IM},
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## π¬ Contact
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* GitHub Issues: [https://github.com/Xiaosheng-Zhao/SpecCLIP/issues](https://github.com/Xiaosheng-Zhao/SpecCLIP/issues)
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* Email: [xzhao113@jh.edu](mailto:xzhao113@jh.edu)
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