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[ascl:2110.013] Nauyaca: N-body approach for determining planetary masses and orbital elements

Nauyaca infers planetary masses and orbits from mid-transit times fitting. The code requires transit ephemeris per planet and stellar mass and radius, and uses minimization routines and a Markov chain Monte Carlo method to find planet parameters that best reproduce the transit times based on numerical simulations. The code package provides customized plotting tools for analyzing the results.

Code site:
https://github.com/EliabCanul/nauyaca
Described in:
https://ui.adsabs.harvard.edu/abs/2021AJ....162..262C and https://ui.adsabs.harvard.edu/abs/2021AJ....162..262C
Bibcode:
2021ascl.soft10013C
Preferred citation method:

https://doi.org/10.5281/zenodo.5230451


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ascl:2110.013
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