Fig. 6.

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Comparison of the stellar mass completeness limits applied to our mock external catalog (red line) with those of the COSMOS2015 (light gray line Laigle et al. 2016) and COSMOS2020 (dark gray line Weaver et al. 2022) catalogs. The stellar mass completeness limits of the deep Euclid catalogs is expected to lie between these two lines.
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