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--- |
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language: |
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- en |
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pipeline_tag: text-generation |
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tags: |
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- llama-3.1 |
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- astronomy |
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- astrophysics |
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- cosmology |
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- arxiv |
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inference: false |
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base_model: |
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- meta-llama/Meta-Llama-3.1-8B |
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--- |
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# AstroSage-Llama-3.1-8B |
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AstroSage-Llama-3.1-8B is a domain-specialized natural-language AI assistant tailored for research in astronomy, astrophysics, and cosmology. Trained on the complete collection of astronomy-related arXiv papers from 2007-2024 along with millions of synthetically-generated question-answer pairs and other astronomical literature, AstroSage-Llama-3.1-8B demonstrates excellent proficiency on a wide range of questions. This achievement demonstrates the potential of domain specialization in AI, suggesting that focused training can yield capabilities exceeding those of much larger, general-purpose models. |
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## Model Details |
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- **Base Architecture**: Meta-Llama-3.1-8B |
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- **Base Model**: Meta-Llama-3.1-8B |
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- **Parameters**: 8 billion |
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- **Training Focus**: Astronomy, Astrophysics, Cosmology, and Astronomical Instrumentation |
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- **License**: Llama 3.1 Community License |
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- **Development Process**: |
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1. Continued Pre-training (CPT) on astronomical literature |
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2. Supervised Fine-tuning (SFT) on QA pairs and instruction sets |
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3. Model merging with Meta-Llama-3.1-8B-Instruct (75% CPT+SFT / 25% Meta-Instruct) |
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## Using the model |
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```python |
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import torch |
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from transformers import AutoModelForCausalLM, AutoTokenizer |
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# Load the model and tokenizer |
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model = AutoModelForCausalLM.from_pretrained("AstroMLab/AstroSage-8b", device_map="auto") |
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tokenizer = AutoTokenizer.from_pretrained("AstroMLab/AstroSage-8b") |
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# Function to generate a response |
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def generate_response(prompt): |
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inputs = tokenizer(prompt, return_tensors="pt").to(model.device) |
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outputs = model.generate( |
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**inputs, |
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max_new_tokens=128, |
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do_sample=True, |
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pad_token_id=tokenizer.eos_token_id, |
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) |
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response = outputs[0][inputs['input_ids'].shape[-1]:] |
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decoded = tokenizer.decode(response, skip_special_tokens=True) |
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return decoded |
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# Example usage |
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prompt = """ |
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You are an expert in general astrophysics. Your task is to answer the following question: |
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What are the main components of a galaxy? |
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""" |
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response = generate_response(prompt) |
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print(response) |
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``` |
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## Model Improvements and Performance |
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AstroSage-Llama-3.1-8B shows remarkable performance improvements: |
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| Model | Score (%) | |
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|-------|-----------| |
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| **AstroSage-Llama-3.1-8B** | **80.9** | |
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| GPT-4o | 80.4 | |
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| LLaMA-3-8B | 72.9 | |
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| Gemma-2-9B | 71.5 | |
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| Qwen-2.5-7B | 70.4 | |
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| Yi-1.5-9B | 68.4 | |
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| InternLM-2.5-7B | 64.5 | |
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| Mistral-7B-v0.3 | 63.9 | |
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| ChatGLM3-6B | 50.4 | |
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The model demonstrates: |
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- Outperformance of all 8B parameter models |
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- Comparable performance to GPT-4o (80.4%) |
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- ~1000x more cost-effective than proprietary models |
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- 8 percentage-point improvement over base Llama-3.1-8b model |
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## Training Data |
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- **Continued Pre-training**: |
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- ~250,000 arXiv preprints (2007-2024) from astro-ph and gr-qc |
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- Astronomy-related Wikipedia articles |
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- Selected astronomy textbooks |
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- Total: 3.3 billion tokens, 19.9 GB plaintext |
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- **Supervised Fine-tuning**: |
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- 8.8 million curated QA pairs |
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- Filtered Infinity-Instruct-7M dataset |
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- Paper summaries and metadata |
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- Total: 2.0 billion tokens, 9.8 GB plaintext |
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## Intended Use |
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- Curiosity-driven question answering |
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- Brainstorming new ideas |
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- Astronomical research assistance |
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- Educational support in astronomy |
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- Literature review and summarization |
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- Scientific explanation of concepts |
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## Limitations |
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- Training data cutoff: January 2024 |
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- As with all LLMs, hallucinations are possible |
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- Limited by 8B parameter size for complex reasoning |
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- Paper metadata not perfectly memorized |
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- Performance primarily validated on multiple-choice questions |
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- Primarily trained for use in English |
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## Technical Specifications |
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- Architecture: Based on Meta-Llama 3.1 |
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- Training Infrastructure: ORNL OLCF Frontier |
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- Hosting: Hugging Face Hub (AstroMLab/AstroSage-8B) |
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## Ethical Considerations |
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While this model is designed for scientific use: |
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- Should not be used as sole source for critical research decisions |
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- Output should be verified against primary sources |
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- May reflect biases present in astronomical literature |
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## Citation and Contact |
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- Corresponding author: Tijmen de Haan (tijmen dot dehaan at gmail dot com) |
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- AstroMLab: astromachinelearninglab at gmail dot com |
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- Please cite the AstroMLab 3 paper when referencing this model |