Example of morpho-kinematic analysis for galaxy ID #4 at z ≈ 0.56. Description is given from left to right. Top row: HST/WFPC2 F814W image, Galfit model (disk+bulge), and residuals, all in the same arbitrary log-scale units. Second row: MUSE [O ii]λ3729 flux map (log scale) with the PSF FWHM size indicated with the black circle, corresponding S/N map (linear scale), and modeled flux map (log scale) from GalPaK^3D. Third row: MUSE observed velocity field from [O ii]λ3729, velocity field of the 2D rotating disk model, associated residual velocity field, and rotating disk model from GalPaK^3D. Bottom: MUSE observed velocity dispersion map from [O ii]λ3729, velocity dispersion map deduced from the 2D velocity field model (which takes into account beam-smearing effect and spectral PSF), convolved associated velocity dispersion map, and velocity dispersion map from GalPaK^3D. In each map, north is up and east is left. The center used for kinematic modeling is indicated with a white cross, the position angle is indicated with a black line that ends at the effective radius.