Fig. 11

Stellar mass distribution of our z> 3 SMGs (green histogram), and z ~ 2 cQGs (2014; red histogram). The blue histogram shows the distribution of the final stellar masses of the z> 3 SMGs by assuming that 10% of their putative gas mass content is converted into stars by the end of the ongoing starburst event, while the magenta dashed histogram represents the final stellar mass distribution where Mgas is based on the mass-metallicity relationship (see text for details). The CO-based gas mass estimate was adopted for AzTEC 1 and AzTEC 3 (Appendix D).
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