pyaneti: Multi-planet radial velocity and transit fitting
Abstract
Pyaneti is a multi-planet radial velocity and transit fit software. The code uses Markov chain Monte Carlo (MCMC) methods with a Bayesian approach and a parallelized ensemble sampler algorithm in Fortran which makes the code fast. It creates posteriors, correlations, and ready-to-publish plots automatically, and handles circular and eccentric orbits. It is capable of multi-planet fitting and handles stellar limb darkening, systemic velocities for multiple instruments, and short and long cadence data, and offers additional capabilities.
- Publication:
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Astrophysics Source Code Library
- Pub Date:
- July 2017
- Bibcode:
- 2017ascl.soft07003B
- Keywords:
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- Software