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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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