Fig. 5.
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Star formation rate as a function of stellar mass, both quantities derived from the SED fitting analysis. The dashed line shows the main-sequence relation from Leslie et al. (2020) and the solid black line the best-fit relation from Speagle et al. (2014). The shaded region indicates the 0.3 dex scatter Leslie et al. (2020), Speagle et al. (2014).
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