Fig. A.2.
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Example of Euclid-like simulated spectra for type 2 AGN in the redshift interval 0.89 ≤ z ≤ 1.83, thus where the Hα complex is within the spectral coverage of the red grism. Spectra are shown at different S/N and noise levels (medium/high on the left and low on the right) for the good (top row), false (mid row), and lost (bottom row) redshift classes (see Sect. 5).
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