versus including (U)LIRGs from Jiao et al. (2017; dark purple) H-ATLAS SMGs (red) and other SMGs from Walter et al. (2011; green). Two of our sources, NAv1.177 (#9) and G12v2.257 (#15) are lacking lens modelling, thus we plot the limit, and the arrows show the direction for lensing correction. A fit to the correlation from the local to high-redshift galaxies is indicated by the blue line, with a slope of 0.94 ± 0.05. We also show a fit with a fixed slope of 1, that is, a linear fit, by the orange dashed line. The source index ID is indicated in Fig. 1 and Table 3.