REBOUND N-body simulation archives used to train and test the machine learning models in Tamayo et al. (2020), 'Predicting the Long-Term Stability of Compact Multi-Planet Systems'. See https://github.
Simulation data are provided on the long-term evolution of the Solar System following a stellar flyby. The simulation begins at 12,000 years after the periastron passage of a perturber star and models
Values of MOID with Earth as a function of the initial (e, inc) values for simulated Venus co-orbital asteroids, used to create Fig. (7) in Carruba et al. 2025, The invisible threat: assessing the col