Fig. 2.
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SFMS of our sample measured using SED fitting (see Section 2.4). The shaded grey regions delineate our stellar mass bins for the stacking analysis. SFRs and the Popesso et al. (2023) SFMS include dust corrections. The dotted line indicates extrapolation. The brown line and orange region delineate the FRESCO Paα SFMS from Liu et al. (2026) and Neufeld et al. (2024), respectively.
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