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Fig. A.1.
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Star-formation rate per unit area as a function of galactic radius. Upper panel: Massive galaxies with EMPIRE data. Middle panel: Massive galaxies without EMPIRE data. Lower panel: Low-mass galaxies. Solid lines show our model SFR prescription (Eq. A.10) and dashed lines Krumholz et al. 2012 SFR prescription (Eq. A.14).
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