ironman is a Python package for jointly fitting in-transit and out-of-transit radial velocities with photometric data. Its main objective is measuring the stellar obliquity of the orbit of a planet using the Rossiter-McLaughlin effect.
- rmfit (pip install rmfit)
- numpy (pip install numpy)
- scipy (pip install scipy)
- pandas (pip install pandas)
- batman-package (pip install batman-package)
- dynesty (pip install dynesty)
- astropy (pip install astropy)
You can install ironman with pip
pip install ironman-package
Or cloning the repository
git clone https://github.com/jiespinozar/ironman
cd ironman
pip install .
To see examples of the usage of this module, see the example notebooks in the Examples folder.
- Example 1: How to fit data with ironman (sky-projected obliquity)
- Example 2: How to simulate data (e.g., for proposals)
- Example 3: How to fit data with ironman (true 3D obliquity)
If you use this code, please cite Espinoza-Retamal et al. 2024
If you use the RM fitting capability, please cite Stefansson et al. 2022 and Hirano et al. 2010
If you use the transit fitting capability, please cite Kreidberg et al. 2015
If you use the RV fitting capability, please cite: Fulton et al. 2018