Fig. 7.
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SFR–M⋆ relation for the lens galaxies and SMGs in our sample. For comparison, the sample of unlensed SMGs is also shown, along with the quiescent (dashed line) and star-forming (dotted line) evolutionary tracks for early-type galaxies from Paspaliaris et al. (2023), and the star-forming main sequence (MS) at z = 2.2 from Speagle et al. (2014) (dash-dotted line). Moreover, the solid lines represent the fits to our data.
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