Fig. A.1.

Kinematic models of five representative galaxies obtained with 3D BAROLO. From left to right: (1) observed and (2) best-fitting model velocity field; the dashed grey line shows the average kinematic position angle, while the bar between the two panels show the colour scheme in both velocity fields. (3) Major axis position-velocity diagram: The data is shown in blue, while black contours enclose the data (grey for negative values) and red contours the best-fitting model. The contour levels are at −2, 2, 4, 8, 16, …times the mean rms in the corresponding data cube. The recovered rotation velocities are shown in yellow. (4) Rotation velocity (red), circular speed (blue) and velocity dispersion (grey) profiles.
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