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.
Credit: Barragán, Oscar; Gandolfi, Davide; Antoniciello, Giuliano
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2019MNRAS.482.1017B