Fig. A.1.
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Comparison of the Lyα properties of AMORE6 with literature samples of galaxies at z > 4. Left: shift of the Lyα peak relative to systemic (dv) versus rest-frame Lyα EW; literature samples from Tang et al. (2024), Saxena et al. (2024), Prieto-Lyon et al. (2025), references for the lensed-galaxies sample in Table A.1. Center: EW(Lyα) versus MUV; AMORE6 is 4 − 5 mag fainter than the comparison average. Right:dv versus FWHMLyα for cases with both measurements.
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