Fig. 5.
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UV β slope vs. ξion(1 − fesc). Lyα-detected galaxies are shown in purple and the photometrically selected sample with no Lyα-detected in gray. As above, error bars are only shown for 30% of the sources for clarity. We add the stacked measurements from Lam et al. (2019) for comparison. We find a very weak trend of increasing ξion with decreasing β, with a linear slope of −0.10 ± 0.06.
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