Projected number density profile of the galactic component derived from the f^(ν) distribution function with fitted parameters for AS1063 and M1206 (see Table 6). The plot shows the data points (in black) derived from photometric data (see Fig. 4) superimposed on the projected number density profile derived from the moments of the distribution function for five choices of the value of the parameter d (see Fig. 16 for the associated anisotropy profile). The value of the parameter A was obtained after a best-fit against the observed profile performed within 2R_hm. Both clusters are well described by the curves associated with a value of d ≈ 10 − 50, confirming the results of Fig. 14.