Fig. A.2.

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Spectra of additional line emitters identified in ALMA datacubes. Left panel: CO(4–3) line of C2 (QSO-SE) detected in the ALMA band 3 spectral scan of C4, corrected for the PB response. Right panel: [CI]609 μm line of C6 identified in the ALMA band 6 datacube. Data and the best-fit model are shown in yellow and red, respectively. The ±1σ RMS noise range of the data is indicated by the gray shaded area. The top scales report the expected line redshifts.
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