Fig. D.1.
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Spectral stacks of CO (olive) and HCN (purple) across NGC 4321 in logarithmically-spaced bins of Σ⋆. The grey-shaded area indicates the velocity-integration window applied to compute the integrated intensities of the stacked spectra. The labelled boxes show the peak intensity and S/N of the integrated intensities of CO and HCN, respectively, for each stacked spectrum.
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