Top: M_B−5 log h₇₀ vs. redshift for our sample of galaxies (crosses) and for zCOSMOS EELGs by Amorín et al. (2015) (filled circles), color coded according to different bins of redshift (0.1–0.3, 0.3−0.5, 0.5–0.7 and 0.7–0.9). The EELG fraction of our galaxies is evidenced by empty circles around the crosses. The B-band luminosities span a wide range, −13 ≤ M_B ≤ −21.5, increasing with redshift. Bottom: Galaxy stellar mass vs. redshift for the same galaxy samples.