CMR of Coma Cluster galaxies (black pentagons) and the red sequence best fit, computed only for the early-type galaxies defined as brighter than H = 14.5 (at the left of the dashed vertical line), with relative scatter (black dotted lines) as provided by Eisenhardt et al. (2007). The overplotted colored points mark the values obtained for the average spectra representative of the high-z cluster members, with the same color code as defined in Fig. 9. Note that for a consistent comparison all the observed H-band magnitudes were rescaled to the corresponding values, as explained in the text. For Coma galaxies a value of = 11.13 was used.