Poster abstract details

Bayesian analysis through Markov-Mote Carlo methods has become a key tool for the exoplanet search and the determination of their orbital parameters. It has proved to be a solid way to to select the appropriate n-planets model and to estimate then the orbital parameters and confidence intervals of a systems even when the data does not cover complete orbital phases. Here we present an in-development code to calculate the orbital parameters and confidence intervals for single planet system (6 parameters) or a double planet system (12 parameters) with future applications in n-planet systems.