Same as Fig. 5 for different migration and damping rates. Rates are shown unchanged in the left panels, Type II migration rate scaled by the factor cos (i_pl) indicated in the middle panels, and no eccentricity and inclination damping considered in the right panels. Two initial inclination values of the planet with respect to the disk plane are also shown (i_pl is fixed to 0° in the top panels and 20° in the bottom panels).