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docs: star-history-style chart (self-hosted; upstream API down for this repo)
Co-Authored-By: Claude Opus 4.8 (1M context) <noreply@anthropic.com>
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‎README.md‎

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@@ -18,13 +18,7 @@ Most LLM-based classification pipelines use a large language model for every sin
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TRACER learns the decision boundary between "easy" and "hard" inputs directly from your LLM's own classification traces. It fits a fast, non-LLM surrogate on the easy partition, gates it with a calibrated acceptor, and defers only the uncertain inputs back to the LLM. Every deferred call produces a new trace, which feeds the next refit - coverage grows automatically over time. The result: **90%+ of classification calls routed to traditional ML, with formal parity guarantees against the teacher LLM and a self-improving routing policy**.
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<a href="https://star-history.com/#adrida/tracer&Date">
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<picture>
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<source media="(prefers-color-scheme: dark)" srcset="https://api.star-history.com/svg?repos=adrida/tracer&type=Date&theme=dark" />
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<source media="(prefers-color-scheme: light)" srcset="https://api.star-history.com/svg?repos=adrida/tracer&type=Date" />
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<img alt="Star History Chart" src="https://api.star-history.com/svg?repos=adrida/tracer&type=Date" width="600" />
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</picture>
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</a>
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<a href="https://star-history.com/#adrida/tracer&Date"><img src="docs/assets/star-history.png" alt="Star History Chart" width="600"></a>
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```bash
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pip install tracer-llm

‎docs/assets/star-history.png‎

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