exoplanet: Case Studies#
These pages contain “case studies” for the exoplanet project. Each case study is an example of a real world
application of the exoplanet library for analyzing data in astronomy. They
are implemented as Jupyter notebooks, and you can download the notebook or
launch it using Binder using the menus at the top
right of each case study.
For more information about exoplanet, check out the main documentation page
at docs.exoplanet.codes.
Tips & tricks
⏰ Note that the runtime for some of these notebooks can be as long as half an
hour, but we’ve tried to keep the studies as self-contained and reproducible
as possible. This computation is generally dominated by the sampling step so
if you want to get a rough sense of the expected runtime for a particular
case study, scroll down to take a look at the progress bar generated by the
call to the sample function.
🐛 If you run into bugs when executing these case studies (or variations on them) on your own computer, open an issue on the exoplanet GitHub repo.
💡 If you have a conceptual issue or a particularly tricky or interesting fit, start a discussion on GitHub so that we can all learn together.
Case studies#
- Radial velocity fitting
- Transit fitting
- Astrometric fitting
- Gaussian process models for stellar variability
- Joint RV & transit fits
- Fitting TESS data
- Quick fits for TESS light curves
- Simultaneous Fitting of a Transit with Stellar Variability
- Datasets and initializations
- A simultaneous transit and Gaussian process model
- Sampling
- Fitting transit times
- Fitting a detached eclipsing binary
- RVs with multiple instruments
- Light curves from multiple instruments
- Main exoplanet docs