Fig. 1.
Comparison between the photometric redshifts (zp) and spectroscopic redshifts (zs) for the simulated Horizon-AGN galaxy sample. Each panel shows a two-dimensional histogram with logarithmic colour scaling and is annotated with both the 1:1 equivalence line (red) and the |zp − zs| = 0.15 (1 + zs) outlier thresholds (blue) for reference. Photometric redshifts are computed using both DES/Euclid (left) and LSST/Euclid (right) simulated photometry, assuming a Euclid-based magnitude-limited sample with VIS < 24.5.
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