Published July 31, 2024
| Version v1.0.2
Software
Open
ironman
Creators
- 1. Pontificia Universidad Católica de Chile
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2.
Millennium Institute of Astrophysics
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3.
University of Amsterdam
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4.
Indiana University Bloomington
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5.
Adolfo Ibáñez University
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6.
Data Observatory Foundation
- 7. El Sauce Observatory
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8.
European Southern Observatory
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9.
Universidade do Porto
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10.
Northern Arizona University
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11.
University of Cambridge
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12.
Instituto de Astrofísica de Andalucía
Description
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.
The version of the code published here is: 1.0.2, which is the one decribed in Espinoza-Retamal et al. (2024). For more recent versions, check GitHub.
Installation
You can install ironman with pip
pip install ironman-package
Or you can download the zip file published here, uncompress it, and
cd ironman
pip install .
Dependencies
- rmfit
- numpy
- scipy
- pandas
- batman-package
- dynesty
- astropy
Examples
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)
Citation
If you use this code, please cite the DOI for this Zenodo repository as well as Espinoza-Retamal et al. (2024)
Files
ironman-1.0.2.zip
Files
(19.5 MB)
| Name | Size | Download all |
|---|---|---|
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md5:acd19288f7f224f30e92523268e21bf2
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19.5 MB | Preview Download |
Additional details
Software
- Repository URL
- https://github.com/jiespinozar/ironman
- Programming language
- Python
- Development Status
- Active