Visual extinction (A_V) toward the jet determined from the observed [Fe II] line ratios with respect to their intrinsic ratios. We calculate the line ratios at peak line flux for spaxels along the northern (blueshifted) jet axis. We use the ratio at peak line flux since the lines are only marginally resolved in wavelength (3 or 4 channels). The observed trends are consistent with the values derived from taking line ratios with zeroth-moment maps which have higher uncertainty due to spaxels that contain faint emission. Vertical dashed lines correspond to the three iron peaks in Fig. 7.