Fig. 4
Completeness of the sample, derived from simulated SEDs with emission lines added. Top panel: completeness as a function of the EW of [OIII] and Hα lines. We reach 50% completeness at around 22 Å in [OIII], 35 Å in Hα. Bottom panel: completeness of the sample, using the same simulations as in the top panel, but plotted as a function of the Hα flux. We reach 50% completeness at around 7.4 × 10−17 erg s−1 cm−2.
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