Fig. C.8.
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Relation between the faint end slope of the luminosity function α and the total star formation rate (upper left panel), total stellar mass (lower left), mean star formation rate surface density (upper right), and mean stellar mass surface density (lower right) of the host galaxies. The black dashed line shows the best fit to the data (bisector fit). The dots in the lower left and right corners show the typical error bar in the data.
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