Fig. B.1.
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LMT/RSR spectra at their native (unbinned) resolution at the position of the detected lines at z = 3.5715 (three first panels; HCN(4-3), 12CO(4-3), and [CI]3P1-3P0 from left to right) and the Lupus molecular cloud (right panel; local 13CO(1-0)). Note that the peak flux density is slightly higher than for the binned spectrum shown in the bottom panel of Figure 3.
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