Same as in Fig. 15, but for the RR Lyrae stars confirmed by the SOS Cep&RRL pipeline for which the colour information is available (1167 sources out of 1986) that are in globular clusters (red points) and dwarf spheroidal galaxies (blue points). Each concentration of red points corresponds to a different GC, the blue overdensity below G ~ 20 mag is due to RR Lyrae stars in the Draco and Sculptor dSphs.