exoplanet: Probabilistic modeling of transit or radial velocity observations of exoplanets

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Ada Coda
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exoplanet: Probabilistic modeling of transit or radial velocity observations of exoplanets

Post by Ada Coda » Tue Oct 29, 2019 10:33 pm

exoplanet: Probabilistic modeling of transit or radial velocity observations of exoplanets

Abstract: exoplanet is a toolkit for probabilistic modeling of transit and/or radial velocity observations of exoplanets and other astronomical time series using PyMC3 (ascl:1610.016), a flexible and high-performance model building language and inference engine. exoplanet extends PyMC3's language to support many of the custom functions and distributions required when fitting exoplanet datasets. These features include a fast and robust solver for Kepler's equation; scalable Gaussian processes using celerite (ascl:1709.008); and fast and accurate limb darkened light curves using the code starry (ascl:1810.005). It also offers common reparameterizations for limb darkening parameters, and planet radius and impact parameters.

Credit: Foreman-Mackey, Dan

Site: https://docs.exoplanet.codes/en/stable/
https://ui.adsabs.harvard.edu/abs/2019arXiv190803222A

Bibcode: 2019ascl.soft10005F

Preferred citation method: Please see citation information here: https://exoplanet.dfm.io/en/stable/tutorials/citation

ID: ascl:1910.005
Last edited by Ada Coda on Mon Feb 17, 2020 12:48 am, edited 1 time in total.
Reason: Updated code entry.

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