Fig. 1.
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Distribution of redshift (first panel), Lyα luminosity (second panel), Lyα line rest-frame FWHM (third panel), and S/N of Lyα line (fourth panel) of the LAE sample. The thick lines present the distributions of the whole galaxy samples in MXDF (blue lines) or MOSAIC (grey lines). The narrow lines show the LAEs at 3 < z < 4, the redshift range of most interest for this work.
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