Fig. B.2.

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LFs for H II regions located in the inner (red colors) and outer disk (blue colors) areas. Galaxies are ordered according to increasing stellar mass from top left to bottom right, and their names are indicated within each panel. The dashed and solid lines indicate the empirical LF and the best fitting model, respectively. The LF slopes are reported in the top-right corner of each panel following the same color scheme. The median galactocentric radius, ⟨rgal⟩, of the H II region parent sample, used to separate inner and outer disks, is indicated below each galaxy name in units of R25.
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