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Fig. 3.

image

Redshift and magnification corrected luminosity distribution of the 152 LAEs used for the LF computation (in blue). The corrected histograms in light red correspond to the histogram of the population weighted by the inverse of the completeness of each source (see Sect. 6.2). The empty bins seen on the redshift histograms are not correlated with the presence of sky emission lines.

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