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Fig. 1


Stellar mass, derived with Eq. (5), as a function of molecular gas mass. The lines show ratios of Mmol /M= 100%, 10%, and 1%, respectively. The objects are color-coded according to the classification of Zucker et al. (2016) with the mid-IR active population in blue and the mid-IR quiescent population in red to follow the optical convention typically adopted in the literature.

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