Fig. D.5.
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Comparison of galaxy SFRs based on 20-cm radio continuum and W3PAH flux densities. The top panel shows the SFR using Eq. 4, which accounts for stars with masses > 5 M⊙, while the bottom panel accounts for stars with masses > 0.1 M⊙. The linear function plotted represents the 1:1 relation; the shaded region indicates the 10% scatter.
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