Fig. 14.
Distribution of AGN-corrected qIR as a function M⋆, colour-coded by redshift (stars). At each M⋆, open squares indicate the median qIR values at z = 1, obtained after propagating the uncertainties of slope and normalisation of the corresponding qIR − z fit and interpolating each at z = 1. These values were fitted with a linear function in log − log space (black dashed line).
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