Fig. 7.
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Far-infrared dust continuum effective radius as a function of the IR luminosity of our galaxies, colour-coded by redshift. Our extreme starburst galaxies agree better with the Reff, FIR–LIR anti-correlation (light-grey shaded area) found by Jin et al. (2022) than with the Reff, FIR–LIR correlation (dark-grey shaded area) of Fujimoto et al. (2017).
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