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Fig. 8.

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Comparison to luminosity functions. The dashed red line shows the selection incompleteness uncorrected luminosity function determined by Hu et al. (2019) using the combined COSMOS and CDFS fields. The dotted green line shows the combined luminosity function from Wold et al. (2022). The black points are the values determined from the LAEs observations in our field. The black line is the Hu et al. (2019) luminosity function scaled to our data. The blue points are the limit-assumption completeness-corrected luminosity function described in Sect. 4.1.

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