Instructions to use KilmaAI/Sadim-77M with libraries, inference providers, notebooks, and local apps. Follow these links to get started.
- Libraries
- Transformers
How to use KilmaAI/Sadim-77M with Transformers:
# Use a pipeline as a high-level helper from transformers import pipeline pipe = pipeline("feature-extraction", model="KilmaAI/Sadim-77M")# pip install -U transformers accelerate # Load model directly from transformers import AutoModel model = AutoModel.from_pretrained("KilmaAI/Sadim-77M", device_map="auto") - Notebooks
- Google Colab
- Kaggle
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Download README.md from KilmaAI/Sadim-77M: direct link, hf CLI and curl.
- Browser
- Download file 2.23 kB
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https://huggingface.co/KilmaAI/Sadim-77M/resolve/main/README.md
- Command line
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hf download hf://KilmaAI/Sadim-77M/README.md
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curl -L -o README.md https://huggingface.co/KilmaAI/Sadim-77M/resolve/main/README.md
2.23 kB
| license: apache-2.0 | |
| datasets: | |
| - samfatnassi/gaia-dr3 | |
| language: | |
| - en | |
| metrics: | |
| - accuracy | |
| library_name: transformers | |
| pipeline_tag: feature-extraction | |
| doi: 10.5281/zenodo.18727667 | |
| # SADIM: Stellar Intelligence Framework | |
| **SADIM-77M** is a specialized AI model trained on the **Gaia Data Release 3 (DR3)** catalog. It bridges the gap between massive raw astronomical observations and actionable scientific insights. | |
| **Research Objectives** | |
| • Galactic Archaeology: Identifying stellar streams and ancient structures. | |
| • Big Data Optimization: Providing an AI-ready interface for 1B+ records. | |
| • Scalability: Real-time stellar analysis for future space surveys. | |
| **Research Link:** https://zenodo.org/records/18727667 | |
| ### 1. Technical Feature Map | |
| The model is designed to process 13 fundamental astronomical parameters: | |
| | Feature Name | Description | | |
| | :--- | :--- | | |
| | **source_id** | Unique Gaia DR3 Identifier | | |
| | **ra / dec** | Celestial Equatorial Coordinates | | |
| | **l / b** | Galactic Coordinates (Disk Alignment) | | |
| | **pmra / pmdec** | Kinematics (Proper Motion Velocity) | | |
| | **d_pc** | Distance in Parsecs (1/parallax) | | |
| | **x, y, z** | 3D Heliocentric Cartesian Mapping | | |
| | **abs_m** | Absolute Magnitude (Intrinsic Brightness) | | |
| | **bp_rp** | Color Index (Temperature Indicator) | | |
| ### 2. When to use the Model vs. the Dataset? | |
| * **Use the SADIM 77 Model:** For fast inference, predicting missing stellar properties, or automating the classification of new astronomical data. | |
| * **Use the Gaia-DR3 Dataset:** For deep-dive research, historical record querying, or training your own custom neural networks. | |
| * **Dataset Link:** [samfatnassi/gaia-dr3](https://huggingface.co/datasets/samfatnassi/gaia-dr3) | |
| ### 3. Quick Start (Python) | |
| Since the dataset contains over **1 Billion records**, we recommend using **Streaming Mode**: | |
| ```python | |
| from datasets import load_dataset | |
| from transformers import AutoModel | |
| # 1. Access the Data | |
| dataset = load_dataset("samfatnassi/gaia-dr3", split="train", streaming=True) | |
| # 2. Load the Model | |
| model = AutoModel.from_pretrained("KilmaAI/SADIM-77M") | |
| # Fetch a sample star | |
| sample_star = next(iter(dataset)) | |
| print(f"Analyzing Star ID: {sample_star['source_id']}") | |