Gas-to-dust mass ratio, δGDR, of CO-detected galaxies with rest-frame λmax ≥ 200μm, computed by combining CO-based gas masses and DL07-based dust masses. Symbols are as in Fig. 13. Left: δGDR as a function of metallicity. The red lines represent the local relation by Magdis et al. (2012) and its 0.15 dex scatter. Right: δGDR as a function of other relevant parameters: redshift z; depletion times based on CO; M∗ (Wuyts et al. 2011a); and .
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