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Fig. 1.

image

fesc(Lyα) as a function of EW0(Lyα) for the galaxies in this sample. Green triangles show fesc(Lyα) in bins of EW0(Lyα). Cyan triangles and magenta stars are the average values for samples at z ∼ 2.2 and z ∼ 2.6 by Sobral et al. (2017) and Trainor et al. (2016), respectively, and the black solid and dashed lines indicate the empirical fit fesc(Lyα) = 0.0048 × EW0 ± 0.05 proposed by Sobral & Matthee (2019).

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