Fig. 4.

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Velocity offset between Lyα and [CII] emission lines as a function of Lyα equivalent width (left) and the absolute UV magnitude (right). We include galaxies from 6 ≲ z ≲ 8, 6.6 ≲ z ≲ 7, and z = 7.2 for comparison (Hashimoto et al. 2019; Endsley et al. 2022; Baier-Soto et al. 2022). The galaxies of this sample are shown in purple in both panels.
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