Fig. 4.
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Size-stellar mass relations. Left: Size-stellar mass relation for galaxies with identified Rnorm. We fit a linear relation to the data and show that a slope of m = 0.34 ± 0.01 is measured, consistent with C22. The shaded grey region shows the 1σ scatter in the linear relation. Right: Size-stellar mass relation using RsSFR, showing the linear fit to the Rnorm-mass relation.
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