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Fig. 7
Distribution of Ly-α luminosities in z = 6.6 LAEs (Kashikawa et al. 2011) (red line). The Ly-α luminosities of the GRB hosts listed in table 4 are represented by the filled gray rectangles. Our limit to the Ly-α luminosity of the GRB 080913 host is indicated by the vertical dashed line.
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