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Fig. 8.

image

AGN-uncorrected qIR evolution as a function of redshift (x-axis) and M (colour bar). Errors on qIR represent the 1σ scatter around the median value, estimated via bootstrapping over LIR and L1.4 GHz. For comparison, other IRRC trends with redshift are taken from the literature (black lines): Bell (2003, dotted); Magnelli et al. (2015, dashed); Delhaize et al. (2017, dot-dashed). Our qIR values still include the contribution of radio AGN. See Sect. 4.1 for details.

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