Top: type selection based on best fitting templates for the “red” sample (left) and the “blue” sample (right) in the CFHTLS Wide. We show the colour distribution (M_u − M_r) as function of absolute magnitude (M_g) and redshift (top to bottom) and number counts for “red” and “blue” objects on the right panels. Bottom: number of red and blue galaxies as function of magnitude and redshift.