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Fig. 1.

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Spectral lines observable within four selected EoR-Spec bands (illustrated by red-shaded regions), and originated from galaxies situated at different redshifts. The dashed numbered lines represent transitions within the CO rotational ladder, with the corresponding numbers indicating the Jup for each specific transition. These CO lines act as the foreground contaminant for the [CII] (red thin dashed line) LIM survey.

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