Fig. 12.
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Hα and [OIII]λ5007 luminosity. The observed luminosities uncorrected for dust are shown as gray dots. The color dots correspond to luminosities de-reddened using AHα and A[OIII] as constrained by the SED fitting with CIGALE. The corrected data is color-coded by the stellar mass. A slope of 0.99 is measured in the dust corrected sample with a 0.39 dex dispersion.
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