sSFR as a function of stellar mass for all the main-ELG contributions, each one represented by contours. In each set of contours, the inner line (outer shade) represents the 68 (95) percent confidence regions. The contours of the SF population at sSFR > 10⁻¹¹ yr⁻¹ (solid black) are broken due to the sharp sSFR cut; those of the passive component (dotted red) are broken due to the very low number density of this population (0.1 percent of the total; see Table 2).