Left: model photocenter displacements for our Keplerian disk model with the disk major axis along a PA of 90°. We impose an opacity field in order to shift the central channels away from the continuum so that they do not overlap. Center: model photocenter displacements for a similar model with an out of plane velocity of 20 km s^-1. We see that the perceived PA of the system axis is offset by a value of 11.2° and that the red-shifted vectors are less displaced from the continuum than their blue-shifted counterparts. Right: a plot of the out-of-plane velocity (v_z) plotted against system axis change (Δθ) for our grid of models showing that the PA offset varies linearly with v_z.