Fig. 15.
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Emission line fluxes measured on stacked mock spectra as a function of stellar mass for the EWS-SFsim selection. From top to bottom, panels display the fluxes of Hα, Hβ, [O III], and [N II] emission lines. The red dotted horizontal line in each panel indicates the flux limit of 2 × 10−16 erg s−1 cm−2 imposed on the Hα line. The layout of the panels is the same as in Fig. 14.
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