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Fig. 3.

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Main spectral features falling in the MUSE spectral range as a function of redshift. Hydrogen Balmer and Lyman lines are shown in black, oxygen lines in blue, absorption lines in orange, and continuum breaks in gray. The background colors indicate the number of bright emission lines simultaneously visible in the MUSE spectral range. As an indication, the spectral window unavailable in AO observations is shown as the horizontal hatched yellow region.

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