Fig. 7.
Distribution of CIII]-λ1908 equivalent width EW(CIII]) in the UV-selected star-forming population at 2 < z < 3.8. The shaded histogram shows the fraction of galaxies with a given EW(CIII]) in bins of δEW = 1 Å (left Y-axis), with Poisson uncertainties from the population statistics indicated as error bars. The cumulative fraction of galaxies with EW(CIII]) above a given EW(CIII]) limit is drawn as the continuous magenta line (values on the right Y-axis), relative to the total population of SFGs at that redshift. About 24% of SFGs with 2 < z < 3.8 present CIII]-λ1908 Å emission with EW(CIII]) ≥ 3 Å.
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