Fig. 20
Relative counts of MUSE HDFS Lyα emitters (in %) versus UV continuum magnitude. Note that the last bin of the histogram contains the 12 Lyα emitters with magnitude 29.25 <I814< 29.75 (taken from Casertano et al. 2000, catalogue) and the 26 MUSE Lyα emitters not detected by HST which have been arbitrarily assigned the average magnitude estimated from the stacked image I814 = 29.5 (see Sect. 5.6).
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