Fig. 12.
Correlation between the star formation rate (SFR) surface density and H2O luminosity surface density in high-redshift SMGs (Yang et al. 2016) (shown in black), including HFLS3 (Riechers et al. 2013) and ADFS-27 (Riechers et al. 2017). The red, blue and green data points represent the R, B, and G components of G09v1.97 from this work. The figure shows a tight linear correlation between ΣSFR and ΣLH2O with a fitted slope of 1.0 ± 0.2, which is valid down to the sub-kpc scales.
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