Fig. 6.
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Comparison of our data, color-coded by the dust attenuation in the UV of each line of sight, with the relation found by Izotov et al. (2018b), shown with the black line. The Green Pea galaxies that the relation was calibrated on are shown with black stars. The more recent measurements of peak separations of low-redshift galaxies by Flury et al. (2022b) are shown with empty blue squares.
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