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Fig. 5.


Redshift dependence of the dust attenuation coefficient, Cbf, applied to the nebular emission in our mock galaxies. Symbols represent the mean value estimated by requiring agreement between the predicted and observed luminosity function for either Hα, Hβ, [O II], or [O III]5007 (violet, blue, green, and red, respectively). The best fit relation is shown by the solid black line.

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