Examples of galaxies from our sample. For each galaxy we show the F814W HST/ACS postage stamp with superimposed the 1″ width slit tilted to follow the galaxy major axis, the continuum-subtracted 2D spectrum, the best-fit kinematic model to the line emission and the residuals between the 2D spectrum and the best-fit model, on the same intensity scale as the 2D spectrum. In the spectra, the vertical and horizontal axes are the spatial position and wavelength, respectively. We show, both for the postage stamp and for the spectrum, the 1″ scale. The first three galaxies are classified as rotation-dominated, whereas the other two galaxies are dispersion-dominated.