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Fig. 6.
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Lyα SB variation for plausible luminosities of the undetected LAEs. We assume that undetected sources cluster like the extrapolated HOD model for log(Lmin/[erg s−1]) = 38.5. Resolved sources cluster like those in the MUSE-Wide sample and the pseudo-NB width is 600 km s−1. We use the Lyα LF from Herenz et al. (2019).
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