Physical properties associated to the SED templates that would be selected as part of our F200W-dropout sample. Top left: redshift and stellar mass. Top right: stellar mass and A_V. Bottom left: stellar mass vs. SFR. Bottom right: redshift and sSFR. For a visual purpose, we associated a log(sSFR/(M_⊙ yr⁻¹)) = −15 to all galaxies with lower sSFR. Colour indicates the density of templates; i.e. number of templates in one bin and corresponding to our F200W-dropout selection respect to the total number of models corresponding to our F200W-dropout selection. SFR and sSFR are discrete as we select for this test a coarser distribution in star-formation histories and ages than the ones used for the SED fitting.