The ALPINE–ALMA [C II] survey - Luminosity function of serendipitous [C II] line emitters at z ∼ 5

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Fig. B.2.

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[C II] LF at z ∼ 5 of the clustered sources after removing the six [C II]–emitters associated to interacting galaxies with the central targets (see Fig. 4). Compared to the LF presented in Sect. 5, this one results in lower values at the faint end.

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