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Fig. 5.

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Comparison between physical properties estimated with and without radio LoTSS photometry, using CIGALE. Left: scatter plots comparing the properties of galaxies with and without radio LoTSS photometry, such as the AGN fraction, AGN luminosity, stellar mass, and SFR. All values are provided in logarithmic scale, with the exception of the fracAGN. Each scatter plot includes a 1:1 reference line, as a dashed red line. Right: bar plots of the differences in the same properties, for each source (numbered in the x axis): SDSS+WISE – SDSS+WISE+LoTSS.

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