Velocity ellipsoids for our minor-axis fields. Correlation between V_l and V_r can be related with bulge triaxility. The color–magnitude selection has been the same shown in Fig. 12 and numbers of the cuts are shown in every plot when present (e.g. for Sagittarius-I the selection is [m555  −  m814 > 1.55 or m814 > 17.8], which includes turnoff and RGB stars). An iterative clipping algorithm to reject stars outside 3.0σ of the velocity ellipsoid was used to rid the sample of stars with a kinematic behavior different than the majority. Each figure includes all the velocity ellipsoids to illustrate the convergence of the method. Enclosed points are those rejected for the final velocity ellipsoid for which the parameters found have been included in Table 4. In addition, for the final selection has been calculated in each case the Spearman’s correlation coefficient r_S and the vertex angle l_v when possible.