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Fig. 1.

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Set of transmission curves 𝒯 = {ugrizYEJEHE} used for the Euclid mission (from left to right). The ugriz passbands are only fiducial, since different sets will be used by Euclid; those represented here are from SDSS. The YEJEHE passbands are from NISP on board Euclid. Only the filter transmissions are shown, without atmospheric, telescope, and detector quantum efficiency effects.

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