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Fig. A.5.
Same as Fig. 15, but swapping the mock photo-z GAMA signals out for a comparison with signals from the best 50% of PAUS photo-z according to the Qz parameter (denoted by ‘Qz50’ in the legends, and open-star data-points). Increases in noise and clustering amplitudes are evident when selecting on photo-z quality in this way.
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