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Fig. 1.

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Redshift distribution (top) and stellar mass as a function of redshift (bottom) of the simulated galaxies obtained with SPRITZ for the Euclid Deep Survey, colour-coded by their SED type (see the legend). Markers represent the median value in the redshift bin and shaded areas the corresponding 68% coverage interval. For details about the mass function distribution at different redshift ranges, we refer the reader to Bisigello et al. (2021).

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