Notes. For each cluster, listed in Col. (1), for the King models, we provide (2) the concentration index c = log (r_tr/r₀) (see Eqs. (A.2), (A.3)) and (5) the truncation radius r_tr, in arcsec; for the f^(ν) models, in Col. (10) the ratio between the anisotropy and the half-mass radius and in Col. (12) the anisotropy radius r_α, defined as α(r_α) = 1 (see Eq. (B.16) for the definition of α), in pc. For both King and f^(ν) models, we list: the core radius R_c (defined in the standard way) in arcsec (Cols. (3) and (9)), the intrinsic half-mass radius r_M, in pc (Cols. (4) and (11), respectively), the total mass M of the cluster (Cols. (6) and (13)) expressed in units of 10⁵M_⊙, the V band mass-to-light ratio in solar units (Cols. (7) and (14)) and the logarithm of the central mass density ρ₀ in M_⊙ pc^-3 (Cols. (8) and (15)).