Morpho-kinematics map for galaxy 121-CGR61. From top to bottom and left to right: HST-ACS image, GALFIT model, HST residuals, CAMEL velocity field, MOCKING velocity field model, velocity field residuals, CAMEL velocity dispersion map, MOCKING beam smearing model (including spectral resolution broadening), and beam smearing and LSF corrected velocity dispersion map. The morpho-kinematics centre and the morphological PA are shown in the HST image and the CAMEL maps as a green cross and a green line whose length corresponds to R₂₂, respectively. The PSF FWHM is indicated as the grey disk in the velocity field. The [OII] surface brightness distribution is overlaid on top of the HST and MUSE [OII] flux maps, with contours at levels Σ_[O II] = 2.5,5,10,20,40 and 80 × 10⁻¹⁸ erg s⁻¹ cm⁻² arcsec⁻².