Fig. 1.
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Representation of interloper galaxies in the (ztrue, zmeas) plane, representative of the Euclid spectroscopic selection. The extent of the vertical axis corresponds to the baseline observed redshift range used for the spectroscopic analysis. The plot refers to one of the EuclidLargeMocks (see Euclid Collaboration: Monaco et al. 2025, and Sect. 4.1).
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