Fig. 14.
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Correlation between SFR and AGN luminosity for estimates derived using CIGALE run with the S12 model and CYGNUS run with the E95 model in four different redshift bins that are size-coded by AGN fraction. We also show the previous work from Harrison et al. (2012), Page et al. (2012), Rosario et al. (2012), Stanley et al. (2015, 2017).
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