Fig. 2
Comparison of QLFs for the redshift bin 3.5 <z< 4.0. Plus signs indicate the QLF reported by Palanque-Delabrouille et al. (2016). Filled circles show the QLF based on the corrected eBOSS dataset. The corrected QLF shows a shallower slope than the original version. The dashed curve is the best-fit PLE+LEDE model reported by Palanque-Delabrouille et al. (2016). The solid curve shows the best-fit PLE+LEDE model based on the corrected dataset.
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