Fig. 5.
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SSA22 protocluster member galaxies (black circles) in the M⋆–SFR plane. The solid line shows the SFMS at z = 3.1 from Speagle et al. (2014). The shaded regions indicate a three times difference from the SFMS. The magenta and cyan circles show 2.8 < z < 3.4 DSFGs from ALMA blank field mosaic (GOODS-ALMA; Franco et al. 2018, 2020) and single-dish follow-up (AS2UDS+AS2COSMOS; Dudzevičiūtė et al. 2020; Simpson et al. 2020; Ikarashi et al., in prep.) surveys.
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