Plots of the dependence of Halo and Disc properties on V_Tan, the on sky velocity. The top panel shows the distribution of V_Tan against V_Toomre, where the horizontal red line depicts the V_Toomre cut used to kinematically define our Halo and Disc Samples. The middle panel shows the purity and completeness of the sample; for the common V_Tan > 200 km s⁻¹ halo selection, the sample is 83% pure and 69% complete. The bottom panel shows the probability of the star belonging to the Disc, as inferred by our method.