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SAJAX — Stellar Activity Grid for Exoplanets in JAX

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SAJAX is a JAX-accelerated reimplementation of SAGE (Chakraborty et al. 2024), a code that models stellar contamination of exoplanet transmission spectra from active regions (ars, faculae) on the stellar surface.

The key innovation over plain SAGE is that SAJAX vectorises the spectral loop with jax.vmap, making it fast on both CPU and GPU without any change to the calling code, and fully differentiable — enabling gradient-based inference with tools like NumPyro or Optax.

Documentation can be found at sajax.readthedocs.io

Installation

pip install sajax

Or in development mode from a local clone. setup_env.sh builds a uv-managed .venv pinned by uv.lock, so every machine gets identical package versions:

git clone https://github.com/SamMerc/sajax.git
cd sajax
./setup_env.sh              # auto-detect: GPU if nvidia-smi sees a device

Useful flags: --cpu / --gpu to override the auto-detection (state --gpu explicitly when provisioning on a GPU-less HPC login node), --docs to add the sphinx dependencies, and --check to report what is already installed.

Run commands in the environment with uv run <cmd> (e.g. uv run pytest), or activate it with source .venv/bin/activate.

Repository layout

sajax/
├── sajax/
│   ├── __init__.py          # public API
│   ├── core.py              # JAX light-curve engine
│   ├── planet.py            # planet orbital dynamics
│   ├── geometry.py          # rotation matrices, coordinate transforms
├── docs/
│   ├── examples/
│   │   ├── introduction.ipynb
│   │   ├── comparison.ipynb
│   │   ├── inference.ipynb
├── tests/
│   ├── test_core.py
│   ├── test_planet.py
├── pyproject.toml
├── .gitignore
└── README.md

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This code creates single- or multi-band light curves for exoplanets transiting active stars

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