Fig. C.1.

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Observed lines of C6H5CN in the 31-50 GHz frequency range towards TMC-1. The abscissa corresponds to the rest frequency assuming a local standard of rest velocity of 5.83 km s−1. The ordinate is the antenna temperature corrected for atmospheric and telescope losses in mK. The red line shows the synthetic spectrum obtained from a fit to the observed line profiles, which provides Tr = 9 ± 0.5 K and N(C6H5CN) = (1.2 ± 0.1) × 1012 cm−2. The blue line shows the synthetic spectrum for a rotational temperature of 6 K and a column density of 1.5 × 1012 cm−2. The rotational quantum numbers are indicated in each panel. Blanked channels correspond to negative features produced in the folding of the frequency switching data. While the blue line produces a very good agreement with the observed intensities for Ka≤4, for higher values of Ka it underestimates the observed intensities by a factor of two.
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