Fig. 5.

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Contribution to the Lyα SB profiles from clustered and undetected LAEs with log(Lmin/[erg s−1]) = 38.5. Differently colored lines correspond to a different assumption for the clustering of undetected LAEs. Detected galaxies are assumed to cluster like those in the MUSE-Wide sample. The data points correspond to the modified stacking experiment of individual LAEs of Wisotzki et al. (2018; see Sects. 2 and 4.4). The triangle denotes an upper limit. We employ a pseudo-NB width of 600 km s−1 and the Lyα LF of Herenz et al. (2019). The shaded gray region shows the typical virial radius of MUSE-Wide LAEs.
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