Fig. B.1.
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Resolved properties measured in 15 − 22″ apertures. Total radio continuum surface brightness at 4.85 GHz as a function of the surface brightness at 100 μm. The black line represents the result of a outlier-resistant linear regression with a slope of 1.02, the dotted lines the scatter of 0.17 dex. NGC 4303, NGC 4535, and NGC 4579 were excluded from the linear regression.
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