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Fig. 2.

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Conditional [C II] LF from the M25 (dashed lines) and M50 (solid lines) simulations at redshifts z = 5 and 3 for central galaxies (left panels), satellites galaxies (middle panels), and all galaxies (right panels). The coloured lines show the CLF of emitters residing in DM halos in different Mhalo bins and the black lines show the total LFs. The dotted grey line in the right panels denotes the luminosity threshold, Lthr, below which the total LFs from two simulations differ significantly due to resolution effects.

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