Currently, a total of 159 globular clusters has been simulated in three Milky Way-like potentials, modeling the process of tidal stripping that these clusters have experienced over the past 5 Gyr, by means of a test-particle approach.
As a result, for all clusters we can predict the distribution of the extra-tidal material in the sky, their proper motions, distances to the Sun, and line-of-sight velocities, as well as Galactocentric positions and velocities.