Fig. 27
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Relative difference of photometric redshift estimated with GalaPy against the real spectroscopic values for the four dusty star-forming galaxies of the Pantoni et al. (2021) sample (green squares), the three quiescent galaxies of the Donevski et al. (2023) sample (blue circles), and the lensed galaxy with upper limits from (Giulietti et al. 2023, red triangle). Markers with error bars trace the median and 68% credible interval of the samples.
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