Fig. 2.
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Stellar mass vs. star formation rate for the sample, derived from the SED reported in the AMUSED database (Bacon et al. 2023), colour-coded by redshift and excluding the two AGNs. The z = 3 SFMS, as derived by Boogaard et al. (2018), is represented by a dashed blue line. The sample shows a slight offset relative to the z = 3 SFMS, but follows the expected linear trend.
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