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Fig. 4.

image

Luminosity function of emission lines. Each panel displays the results for a different emission line from top to bottom and from left to right: Hα, [O II], Hβ, and [O III]5007. Shown in each panel are the various observational estimates (cf. Sect. 3.2 and Appendix B) at different redshifts, colour-coded as shown in each legend. Dashed and solid lines display the results from our mock galaxy catalogue before and after applying an empirical model for dust attenuated, respectively. This dust model has been calibrated to improve the agreement between the observations and our predictions.

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