Fig. 6.

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AGN effect on [C I] emission: [C I](3P1 − 3P0) and [C I](3P2 − 3P1) L′ luminosities and their ratio as a function of the IR luminosities from the star-forming component LIR, SFR. Filled and empty blue circles mark our sample at z ∼ 1.2 as in previous figures. Squares indicate the sample in Valentino et al. (2018), selected at similar redshift and luminosity.
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