Fig. A.1
Comparison between the single-dish IRAM 30 m spectra (black histogram) published by Pacheco-Vázquez et al. (2015) and NOEMA interferometric spectra (red points). We note that the 30 m observations were performed using the wobbler switching procedure and the cloud emission is subtracted with the OFF position. The absence of missing flux does not imply the absence of an extended component.
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