Photometric and kinematic fits for three globular clusters of the sample. Each cluster is representative of its relaxation class as identified by the core relaxation time T_c (for NGC 6341, log T_c ≈ 7.96; for NGC 6656, log T_c ≈ 8.53; for NGC 2419 log T_c ≈ 9.87). The curves represent the surface brightness profile (left panels) and velocity dispersion profile (right panels) calculated by means of dynamical models. In particular, dotted lines correspond to King models; dashed lines to non-truncated f^(ν) models, and solid lines to models. In all panels, the dots are the observed data. For each datapoint, errors are shown as vertical bars; in the case of the velocity dispersion profile, the horizontal bars indicate the size ofthe radial bin used to calculate each data point. The King profiles, f^(ν) profiles, and observed data are taken from ZBV12.