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Fig. 10


Relationship of SFR with [CII] (left panel) and [OI] (right panel) luminosity of LBAs. In the left panel we add samples of massive MS (M ~ 1010M) galaxies at z ~ 0.3 from Ibar et al. (2015) and of ULIRGs at z ~ 0.2 from Magdis et al. (2014). In the LBA and the Ibar et al. samples, we assign different colors according to galaxy BPT classifications. The green box indicates the position of four MS SFGs at redshift 7 published by Pentericci et al. (2016). The lines indicate the relationships found by De Looze et al. (2014) for samples of different types of local galaxies (solid colored lines, as shown in the legend) and the relation followed by a sample of normal local spirals presented in Herrera-Camus et al. (2015; dashed black line). The SFRs of all galaxies have been derived from LIR and a Kroupa IMF to be consistent with the derivation of De Looze et al. (2014).

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