Fig. 2
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Distribution of galaxy magnitudes in the Int catalogues (left) and the SED catalogues (right) for the various optical and NIR bands used herein. Vertical dashed lines indicate the expected 10σ sensitivity of the Euclid Wide and Deep Surveys in the IE, YE, JE, and HE bands. In all bands, only photometry with a signal-to-noise ratio ≥3 is included.
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