Number density (gray scales) of galaxies in the M_NUV − M_r versus M_r − M_J plane at z_r,1 =  [0.2,0.65) (top panel) and z_r,2 =  [0.65,0.95) (bottom panel). Dashed and solid contours are the number density of early (S_type ≤ 8) and late (S_type > 8) spectro-photometric types, respectively. We show those galaxies detected in the K band. The number of sources in each interval, n_gal, is labeled in the panels. The black solid line is the condition M_NUV − M_r = 4.25 that we use to split our galaxies into red and blue. (A colour version of this plot is available in electronic form.)