Fig. 1
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Summary of Euclid’s ability to identify bright MUV < −22 LBGs detectable only in NISP (or VIS/IE dropout) from the ERO data of Abell 2764 and Abell 2390. Model spectra of an LBG at z = 7, 8, and 9 are generated with python-FSPS. Euclid IE, YE, JE, and HE transmission curves are normalised such that their peak coincides with the selection function adopted in this work.
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