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[ascl:1707.003] pyaneti: Multi-planet radial velocity and transit fitting

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.

Code site:
https://github.com/oscaribv/pyaneti
Appears in:
http://adsabs.harvard.edu/abs/2016AJ....152..193B http://adsabs.harvard.edu/abs/2017arXiv170200691B http://adsabs.harvard.edu/abs/2017AJ....153..130E http://adsabs.harvard.edu/abs/2017AJ....153..131N http://adsabs.harvard.edu/abs/2017A%26A...601A.128N http://adsabs.harvard.edu/abs/2017arXiv170200691B http://adsabs.harvard.edu/abs/2017arXiv170504163G http://adsabs.harvard.edu/abs/2017arXiv170408284F
Bibcode:
2017ascl.soft07003B

ascl:1707.003
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