Fig. E.1.
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a: left: [OIII]52 μm line luminosity versus the total IR luminosity. b: centre: [NIII]57 μm line luminosity versus the total IR luminosity. c: right: [OI]63 μm line luminosity versus the total IR luminosity. In the figures, blue squares represent AGN while red stars show the SFG sample. The dashed blue line represents the linear correlation for the AGN sample, the dot-dashed red line shows the relation for SFG, and the black solid line the relation shows the relation obtained by Spinoglio et al. (2012, 2014).
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