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Fig. 2.

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KDE-filtered redshift distribution of the 695 LAEs of our sample, taken from 68 fields of the MUSE-Wide survey. The sample spans a redshift range of 3.3 < z < 6. The kernel is chosen to be a Gaussian with standard deviation σz = 0.005. The expected z-distribution of an unclustered population following the Lyα luminosity function of Herenz et al. (2019) and the selection function of the MUSE-Wide survey is overplotted in red.

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