Fig. 5.
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Observed [C II] line profiles obtained with ALMA for sources C10, C14, and C17 (see, Hill et al. 2020), which overlap spatially with the Lyman-α Blob obtained with MUSE (see Fig. 2). The scaled Lyman-α profile is shown in orange for reference. The velocity scale refers to z = 4.304 for all emission lines. The Lyman-α spectra is not corrected by Verhamme et al. (2018).
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