Top panels: probability of stars of belonging to the ks_thick (red), ks_thin (blue) disc, or ks_halo as a function of fraction of stars (left) and a zoom-in of a small fraction of stars to help visualise the halo probabilities (right). Middle panels: velocity components U (left), V (middle), and W (right) distributions of selected ks_thick (red) and ks_thin (blue). Bottom panels: distribution of the heliocentric radius projection over the Galactic plane, R, (left), and distance from the plane, z, (right) of the selected ks_thick (red) and ks_thin (blue).