Fig. E.2.

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Observed transitions of C5N− in TMC-1. Quantum numbers are indicated at the top right of each panel. The abscissa corresponds to the rest frequency adopting a velocity for the source of 5.83 km s−1 (Cernicharo et al. 2020c). The ordinate is the antenna temperature, corrected for atmospheric and telescope losses, in mK. Blank channels correspond to negative features produced when folding the frequency-switched data. The red line shows the modelled spectra for these lines (see App. E).
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