Fig. 8.
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Gas-depletion time of the HLS sample based on the molecular mass from Rayleigh-Jeans dust emission and the star formation rate from far-IR luminosities. The dashed red line shows the redshift evolution of the gas-depletion time of main-sequence galaxies from Tacconi et al. (2020). The gray dots show the gas-depletion time of z > 2 SMGs based on the data summarized in Dunne et al. (2022).
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