Joint Fit Rossiter McLaughlin Data with photometry and out-of-transit radial velocities
Project description
Ironman
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 canonical Rossiter-McLaughlin effect.
Dependencies
Required packages:
- numpy (pip install numpy)
- scipy (pip install scipy)
- pandas (pip install pandas)
- batman-package (pip install batman-package)
- rmfit (and its dependencies, install from here: https://github.com/gummiks/rmfit)
- dynesty (pip install dynesty)
- astropy (pip install astropy)
Installation
You should be able to do the following:
git clone https://github.com/jiespinozar/ironman
cd ironman
pip install .
Examples
To see examples of the usage of this module, see the example notebooks.
- Example 1: How to fit data with ironman
- Example 2: How to simulate data (e.g., for proposals)
Citation
If you make use of this code, please cite Espinoza-Retamal et al 2024
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