Fig. 2.
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Comparison of the unobscured SFRUV (uncorrected for dust attenuation) and obscured SFRIR of our galaxies, colour-coded by redshift. The majority of our galaxies is dominated by the unobscured SFRUV, such that the corresponding obscured fractions of star formation range between fobscured < 14% and 42%, and is above 50% for three galaxies only. The dashed line traces the one-to-one relationship.
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