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Fig. 3.

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Comparison of the AB magnitudes of PN candidates from H+2020 with those from the e2PN.S survey. The colour coding is the same as in the left panel of Fig. 1. The grey shaded region indicates where 99% of Subaru sources would fall if one plotted two independent measurements of their magnitudes mAB, Subaru against each other H+2020. The error bar in the lower right corner denotes the typical magnitude uncertainty of the PN.S.

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