Relative importance of the features of our energy and direction RFs. The energy regression is mostly related to the total light of the fit model and to the temporal development that indirectly relates to the impact parameter, and thus the distance between the telescope and the EAS. The displacement regressor, which gives the angular separation between the source and the image centroid, has a strong dependence on the model length and temporal development. Finally, the displacement classifier, determining which side of the image centroid the source is located on, is largely dominated by the LH fit, Ψ, which combines information on the orientation of the model and the direction of temporal development.