Comparison of the gas kinematic major-axis PA between this work (PA) and C16 (PA), as a function of the galaxy’s ellipticity measured from the MUSE white light image. Our results are based on the gas kinematics of the brightest emission line (see Table 2) derived with pPXF and the method presented in Krajnović et al. (2006). Values from C16 were measured with CAMEL (Epinat et al. 2012) using the group of lines ([OIII]λλ5007, 4959, Hβ). We find good agreement within the (large) uncertainties, with a median ΔPA_gas of ≈7° ± 31°, and consistent measurements at less than 20° for 8/10 galaxies (see histogram). The galaxy ID numbers are indicated above each point.