Fig. 27.
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Simulated spectrum of a typical galaxy (in terms of mass and star formation rate) from the Euclid weak lensing population at z = 1 (D. Masters, priv. comm.), overlapping the IE, YE, JE and HE bands. The Vera C. Rubin Observatory photometric bands (u, g, r, i, z, y) are also shown, highlighting the importance of the ground-based data to the photometric redshift derivation as the 4000 Å break falls within the i band. The total sensitivity for the ground is given at 1.2 airmass.
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