Redshift distributions of SFR a), stellar mass b), specific SFR c), and HST-ACS I-band half-light radii d). Symbols and colors are the same as in Fig. 3. The normalized distribution of EELGs (filled) and SFGs (black) for each property are shown in the histograms to the right of the panels. Solid, dashed, and dotted lines in b) show the logarithmic fitting to the limiting masses of the star-forming sample for levels 25%, 50%, and 75% of completeness, respectively. The EELGs are small galaxies forming the low end of stellar mass and the high end of sSFR distributions of SFGs in zCOSMOS up to z ~ 1.
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