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Fig. 3.
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Lyα velocity offset (ΔvLyα) with respect to the [C II] line as a function of Lyα equivalent width (left) and absolute UV magnitude (right) observed in star-forming galaxies at 5 < z < 8 (gray circles; Hashimoto et al. 2019). The tentative detection (3σ) of GN-108036 is shown in both panels with a pink diamond.
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