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README.md
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---
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license:
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tags:
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---
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should probably proofread and complete it, then remove this comment. -->
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- learning_rate: 2e-05
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- train_batch_size: 24
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- eval_batch_size: 8
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- seed: 42
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- distributed_type: multi-GPU
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- num_devices: 7
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- total_train_batch_size: 168
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- total_eval_batch_size: 56
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- optimizer: Adam with betas=(0.9,0.999) and epsilon=1e-08
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- lr_scheduler_type: cosine
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- lr_scheduler_warmup_ratio: 0.03
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- num_epochs: 1.0
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- Tokenizers 0.19.1
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license: mit
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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
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- astronomy
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- astrophysics
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- arxiv
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inference: false
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base_model:
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- meta-llama/Llama-3-8b-hf
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# AstroLLaMA-3-8B-Base_AIC
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AstroLLaMA-3-8B is a specialized base language model for astronomy, developed by fine-tuning Meta's LLaMA-3-8b architecture on astronomical literature. This model was developed by the AstroMLab team. It is designed for next token prediction tasks and is not an instruct/chat model.
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## Model Details
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- **Base Architecture**: LLaMA-3-8b
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- **Training Data**: Abstract, Introduction, and Conclusion (AIC) sections from arXiv's astro-ph category papers (from arXiv's inception up to January 2024)
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- **Data Processing**: Optical character recognition (OCR) on PDF files using the Nougat tool, followed by summarization using Qwen-2-8B and LLaMA-3.1-8B.
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- **Fine-tuning Method**: Continual Pre-Training (CPT) using the LMFlow framework
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- **Training Details**:
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- Learning rate: 2 × 10⁻⁵
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- Total batch size: 96
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- Maximum token length: 512
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- Warmup ratio: 0.03
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- No gradient accumulation
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- BF16 format
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- Cosine decay schedule for learning rate reduction
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- Training duration: 1 epoch (approximately 32 A100 GPU hours)
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- **Primary Use**: Next token prediction for astronomy-related text generation and analysis
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- **Reference**: Pan et al. 2024 [Link to be added]
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## Generating text from a prompt
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[The code example remains the same as in the previous version]
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## Model Limitations and Biases
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A key limitation identified during the development of this model is that training solely on astro-ph data may not be sufficient to significantly improve performance over the base model, especially for the already highly performant LLaMA-3 series. This suggests that to achieve substantial gains, future iterations may need to incorporate a broader range of high-quality astronomical data beyond arXiv, such as textbooks, Wikipedia, and curated summaries.
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Here's a performance comparison chart based upon the astronomical benchmarking Q&A as described in [Ting et al. 2024](https://arxiv.org/abs/2407.11194), and Pan et al. 2024:
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| Model | Score (%) |
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|-------|-----------|
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| **AstroLLaMA-3-8B (AstroMLab)** | **72.3** |
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| LLaMA-3-8B | 72.0 |
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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 | 64.0 |
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| Mistral-7B-v0.3 | 63.9 |
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| ChatGLM3-6B | 50.4 |
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As shown, while AstroLLaMA-3-8B performs competitively among models in its class, it does not surpass the performance of the base LLaMA-3-8B model. This underscores the challenges in developing specialized models and the need for more diverse and comprehensive training data.
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It's worth noting that the AstroLLaMA-3-8B-Plus which we will release in the next model release addresses these limitations by expanding beyond astro-ph data.
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## Ethical Considerations
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While this model is designed for scientific use, users should be mindful of potential misuse, such as generating misleading scientific content. Always verify model outputs against peer-reviewed sources for critical applications.
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## Citation
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If you use this model in your research, please cite:
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```
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[Citation for Pan et al. 2024 to be added]
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```
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