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Fig. 4.

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Radiative transfer models for LAEs in the literature. The systemic redshift is fitted between the peaks for every profile except for CDFS-1, suggesting that this source is indeed different from other LAEs. We also note that the peaks in CDFS-1 are visibly narrower than those of its counterparts. Vertical dashed black and red lines mark the zero and the best-fit expansion velocities, respectively.

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