picaso enables the: 1) computation of exoplanet and brown dwarf spectroscopy in transmission, emission or reflected light, 2) 1D climate modeling of brown dwarfs and exoplanets, 3) fitting spectroscopic data to models with grids and retrievals.
- Website: https://natashabatalha.github.io/picaso/index.html
- Installation: https://natashabatalha.github.io/picaso/installation.html
- Tutorials: https://natashabatalha.github.io/picaso/tutorials.html
- Workshops: https://natashabatalha.github.io/picaso/workshops.html
- Source code: https://github.com/natashabatalha/picaso
- Contributing: https://natashabatalha.github.io/picaso/contribution.html
- Bug reports: https://github.com/natashabatalha/picaso/issues
- Physics help: https://natashabatalha.github.io/picaso_dev
- What to cite: https://natashabatalha.github.io/picaso/credit.html
- Reflected Light Spectroscopy of planets
- Thermal Emission Spectroscopy of planets and brown dwarfs
- Transit Spectroscopy of planets
- Phase Curves of planets
- 1D Climate modeling of planets and brown dwarfs
- Fitting models to data
Contributions are always welcome no matter the code level you are at. We value anything from small typos in our documentations page to larger feature changes. We follow the all-contributors specification. This means that contributions of any kind welcome! If you are a new to GitHub and conda environments you can read our instructions here: https://natashabatalha.github.io/picaso/contribution.html
Additionally all contributors agree to adhere to this project's code of conduct
Anyone is free to use the contributor bot to add their contribution. Simply comment on an issue or pull request with:
@all-contributors please add @<username> for <contributions>
Thanks goes to these wonderful people (emoji key):
