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A Python package for fitting secular evolution models to exoplanet transit and radial velocity observations, and interpreting results in the context of various theoretical predictions.

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OrbDot

Author:Simone R. Hagey
Version:1.0.0
Documentation Status License Information

Welcome to OrbDot!

OrbDot is a Python package that uses observational data to study the secular (long-term) evolution of exoplanet orbits. Powered by nested sampling algorithms, it fits evolutionary models using any combination of transit and eclipse timing, radial velocities, and transit durations. OrbDot can further aid in the interpretation of model fitting results by generating reports of model comparisons, derived tidal decay parameters, predicted precession rates, implications for planetary companions, and more.

The documentation, including examples, are hosted on Read the Docs.

Installation

See the installation guide for instructions on installing OrbDot and its dependencies.

Citing OrbDot

Please see the citation instructions if you are using OrbDot in your research.

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A Python package for fitting secular evolution models to exoplanet transit and radial velocity observations, and interpreting results in the context of various theoretical predictions.

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