Additional observables obtained from the DISCMINER analysis of the discs around MWC 480, HD 163296, AS 209, (IM Lup and GM Aur in next page) as traced by ¹²CO, 13CO, and C¹⁸O. Top row: Rotation curves computed from azimuthal averages of deprojected line-of-sight velocities. For reference, the grey dashed line in each panel is the Keplerian rotation curve of the best-fit model found for ¹²CO. Second row: Azimuthally averaged profiles of line widths, defined as the standard deviation of Gaussians fitted to the data line profiles. For reference, the purple dashed line in each panel represents the thermal broadening computed at the ¹³CO peak brightness temperature. Third row: Azimuthally averaged profiles of peak intensities converted to brightness temperatures using the Rayleigh-Jeans law. Bottom row: Elevation of upper and lower emission surfaces. Apart from intensity profiles, all panels in each row share the same x and y-axis extent. Vertical dashed, solid, and dotted lines mark the radial location of dust gaps, rings, and kinks observed in the channel maps of ¹²CO, respectively.