Fig. 3.
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Main properties (photometric redshift, stellar mass, SFR, and dust extinction) of our RS-NIR-faint galaxies. We show – for comparison – the same properties computed by Gottumukkala et al. (2024) and McKinney et al. (2025) for their sample of JWST-selected and SCUBA-selected DSFGs as the green and orange solid lines, respectively. To allow a fair comparison, we only include the sources by Gottumukkala et al. (2024) with F150W > 26.1 mag and exclude the sources flagged as possible AGN.
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