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Fig. 9.

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Molecular gas content of the 13 ALMA sources with CO emitter counterparts, obtained from 1.2 mm fluxes and CO(1–0) luminosities, respectively. Different αCO values of 0.8 and 3.6 M (K km s−1 pc2)−1 are adopted to convert the CO luminosities to molecular gas masses and marked as red and orange, respectively. The gas measurements by using the αCO assigned for each source following Jin et al. (2021) are shown in blue dashed lines.

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