Fig. 10.

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Diagram used to asses the completeness of the EELG sample. We plot the number of galaxies per bin of log(EW[OIII]) as a function of log(EW[OIII]). We overplot the linear fits to the data considering three different limits in the lower end, from 2.45 log(Å) (black line), 2.55 (red), and 2.65 (green). The points considered in at least one of the fits are shown in a darker shade of gray.
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