Pyaneti: a fast and powerful software suite for multi-planet radial velocity and transit fitting
Earth and Planetary Astrophysics
2018-09-19 v1 Instrumentation and Methods for Astrophysics
Data Analysis, Statistics and Probability
Abstract
Transiting exoplanet parameter estimation from time-series photometry and Doppler spectroscopy is fundamental to study planets' internal structures and compositions. Here we present the code pyaneti, a powerful and user-friendly software suite to perform multi-planet radial velocity and transit data fitting. The code uses a Bayesian approach combined with an MCMC sampling to estimate the parameters of planetary systems. We combine the numerical efficiency of FORTRAN, the versatility of PYTHON, and the parallelization of OpenMP to make pyaneti a fast and easy to use code. The package is freely available at https://github.com/oscaribv/pyaneti.
Cite
@article{arxiv.1809.04609,
title = {Pyaneti: a fast and powerful software suite for multi-planet radial velocity and transit fitting},
author = {O. Barragán and D. Gandolfi and G. Antoniciello},
journal= {arXiv preprint arXiv:1809.04609},
year = {2018}
}
Comments
15 pages, 6 figures, 2 tables. Accepted for publication in MNRAS