Fig. 21
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Colour transformation between DES and Euclid NISP photometry for Dorado (top) and between PS1 and Euclid NISP photometry for Perseus (bottom). The figure setup is as in Fig. 19. Extinction is applied to the synthetic magnitudes (AV = 0.05 mag in the case of Dorado, AV = 0.45 mag in the case of Perseus), and a typical extinction vector for AV = 0.5 mag is also shown.
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