Fig. 12.
Observed fesc(Lyα) (left) and 
(right) versus the dust extinction of the stellar continuum with logarithmic y-axes. We included the shape of the dust attenuation curve at the wavelength of interest (either Lyα or LyC) with a dashed line. The correlation between the escape fractions of Lyα and LyC photons and the respective dust attenuation curve is significant at 3σ.
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