Observations, models, and residuals of the flux, velocity, and velocity dispersion from the [O III]5008 Angstrom line. Models are shown for each component (Cols. 2 to 6) and for the five components together (Col. 7). Residuals (Col. 8) are the observation (Col. 1) minus the model (Col. 7). On the velocity maps of individual galaxies, iso-LOS velocity curves are represented in dashed (solid) black lines for values below (above) the systemic velocity of each galaxy.