Fig. C.14.
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Relation between L(Hα)3/L(Hα) (contribution of the brightest three H II regions to the total Hα luminosity of the galaxy) and the total star formation rate (upper panel) and total stellar mass (lower panel) of the host galaxies. The black dashed line shows the best fit to the data (bisector fit), while the black dot the typical error in the data.
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