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Fig. 1.

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Galaxies studied in this work: Lyα-detected galaxies (in purple) and galaxies photometrically selected (with no Lyα-detected, in gray). Top: Distribution of redshifts for the spectroscopic and photometric samples. We show the spectroscopic redshift, where available, or the peak photometric redshift. Bottom: UV magnitude distribution for our sample. We find a median value of −18.14 ± 1.58, with no statistically significant difference between the two samples.

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