Fig. 1.
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Metallicity, stellar mass, and specific SFR distributions of the ALMA targets (black open circles) compared to the parent MOSDEF sample at z = 1.5 − 2.5. Solar metallicity is shown with the grey line in the upper panel. The star-forming main sequence at z = 2.0 − 2.6 (Shivaei et al. 2015) is shown by the dashed line in the lower panel.
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