Fig. B.2.

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Illustration of inferred power-law distributions for typical subsolar metallicity (on top) and super-solar metallicity (on bottom) galaxies. For each metallicity case we show the individual draws for the integration weight (Φ(p); Eqn. 2) on top and the PDF for the lower and upper boundaries for integration (pmin, max; gray) and the average parameter value (pavg; red) the bottom).
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