Star formation rate (SFR) vs. total stellar mass (M_*), tracing the MS of galaxies, where SFR_tot = SFR_Hα corrected for dust reddening. The brown filled circles represent the data used in this work. The dashed-dotted orange line shows the least-squares fit to our data, and the blue line shows the Speagle et al. (2014) MS relation at z ∼ 0.85. The shaded blue region represents the MS limit between redshift 0.7 ≤ z ≤ 1.2, which includes 0.3 dex uncertainty at each redshift.