Our sample of cluster and field galaxies studied following the methods explained in Sect. 3 and presented in the same order as in Table A.2. The first column shows the HAWKI K-band or HST-F850LP image centered on the target galaxy. The second column displays the residuals after subtracting the 2D model of the galaxy. The third column presents the synthetic velocity field based on the observed structural parameters after fitting the simulated rotation curve to the observed curve. The black lines mark the position of the edges of the slit. The fourth column displays the rotation curve (black points) in the observed frame, and the fitted simulated RC (red line).