Fig. 3.
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Uncertainties of the photometric redshifts for the 0.6–0.8 redshift range. First (leftmost) panel: Distribution for BASS/MzLS. Dotted black lines show the smoothed interpolation function used for the photometric redshift painting. Second panel: Same but for DECaLS within the NGC. Third panel: Same but for DECaLS within the northern part of the SGC. Forth panel: Same but for DECaLS within the southern part of the SGC.
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