TRADES (TRAnsits and Dynamics of Exoplanetary Systems) simultaneously fits observed radial velocities and transit times data to determine the orbital parameters of exoplanetary systems from observational data. It uses a dynamical simulator for N-body systems that also fits the available data during the orbital integration and determines the best combination of the orbital parameters using grid search, χ2 minimization, genetic algorithms, particle swarm optimization, and bootstrap analysis.
https://ui.adsabs.harvard.edu/abs/2014A%26A...571A..38B , https://ui.adsabs.harvard.edu/abs/2017AJ....153..224M , and https://ui.adsabs.harvard.edu/abs/2019MNRAS.484.3233B