Fig. 5.

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Overview of the Lyman α emission lines of the 35 LAEs with the highest measured EW0, sorted by EW0 in descending order (left to right, top to bottom). We note that the y-axis shows the flux normalised to the maximum of each peak for better comparison. The vertical dashed lines indicate the positions of the Lyman α lines and the blue bump if there is one. The grey shaded area shows the standard deviation from the MUSE spectra. The shown objects are taken both from the MUSE-Wide and -Deep surveys and have been continuum subtracted.
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