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update models
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j-faria committed Jan 29, 2024
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Expand Up @@ -7,20 +7,21 @@ a given dataset. The models share a common organization, but each has its own
parameters, priors, and settings.

- [RVmodel][kima.RVmodel]
models the RVs with a sum-of-Keplerians
Models the RVs with a sum-of-Keplerians

- [GPmodel][kima.GPmodel]
models the RVs with a sum-of-Keplerians plus a correlated noise component
Models the RVs with a sum-of-Keplerians plus a correlated noise component
given by a Gaussian process

- [RVFWHMmodel][kima.RVFWHMmodel]
models the RVs together with the FWHM as an activity indicator, including a
Models the RVs together with the FWHM as an activity indicator, including a
Gaussian process for the activity signal

- [BINARIESmodel][kima.BINARIESmodel]
this includes tidal and relativistic effects as well as apsidal precession of
This includes tidal and relativistic effects as well as apsidal precession of
the binary’s orbit (applicable for circumbinary planets), and can also fit
double-lined binary data.
double-lined binary data. More details are available in
[Baycroft et al. (2023)](https://ui.adsabs.harvard.edu/abs/2023MNRAS.521.1871B/abstract){:target="_blank"}.

- TRANSITmodel (coming soon)
- GAIAmodel (comming soon)
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