Fig. 9.
Left panel: cumulative distribution of Lyα REW P(> REW) for the complete sample of redshift 6 and 7 galaxies in red and black, respectively. The lines are the best fit exponential functions of the two distributions. Right panel: same distribution but only for galaxies with MUV > −20.25 (the faint sample). The dashed line indicates the previously adopted fit to the distribution at z ∼ 6 (e.g., Dijkstra et al. 2011; LP14).
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