Fig. C.1

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CCFs for 12CO, 13CO, ,
, HF, and Ca abundances. The CCFs were calculated for each order–detector pair and summed over all orders and detectors, after which they were converted to S/Ns by dividing by the standard deviation of the CCFs in the range |vrad| > 100 km s−1. The different colours represent the different targets, J0835, J0501, and J0500. The peaks at vrad = 0 km s−1 are a result of the cross-correlation being performed on the observed spectrum centred in its rest frame. We indicate the peak S/N values in units of σ for each species and BD in the upper-right corner.
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