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Fig. 7.

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Stacked spectra around the CO(1−0) emission line for the three bins defined in Sect. 4.2: Low-mass galaxies (log M*/M⊙ < 10.5), massive galaxies (log M*/M⊙ > 10.5) excluding AGN candidates, and massive AGN candidates. We achieve S/N ≈ 8, 10 and 13 for our stacked measurements respectively.
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