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Fig. B.4.


Luminosity function of [O II] line at 18 different redshifts. Shown are the comparisons with the observational works of Ly et al. (2007), Takahashi et al. (2007), Gilbank et al. (2010), Drake et al. (2013), Ciardullo et al. (2013), Comparat et al. (2016), and Hayashi et al. (2018). The black dots represent the observational data, while the solid orange line and grey dashed line the predictions of our mocks LF with and without dust attenuation.

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