[OIII] EW of the EELG (color dots) and candidate (gray dots) samples as a function of stellar mass. We plot the galaxies in the EELG sample according to their morphology in different colors: red corresponds to compact, green to semicompact, and blue to extended objects. In addition, we overplot linear relations from Khostovan et al. (2016) at different redshifts (black at z ∼ 0.84, blue at z ∼ 1.42, pink at z ∼ 2, and orange at z ∼ 3.24). The linear relations are plotted in as continuous lines in the mass ranges in which they were defined, and as dashed lines in their extensions to lower masses.