Fig. 6

CMD of the ALHAMBRA galaxies at different redshift bins. The filters F365W and F582W, both in Vega magnitudes, are used as a proxy for the Johnson filters U and V. Redder and bluer colours indicate regions of the CMD with higher and lower galaxy densities, respectively. The dashed red line is the colour–magnitude relation that splits the RS from the blue cloud for the mean redshift of the bin, as expressed in Eq. (21).
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