Mass–size relation of star-forming members (blue), quiescent members (red), field SFGs (black), and field QGs (green). Power-law fits to SFG members and field SFGs are shown with blue solid and black dotted lines respectively, with the fit uncertainty of SFG members shown as shaded region. Mass–size relations of late type galaxies from Ward et al. (2024, green line) and quiescent galaxies from Ito et al. (2024, red line) are overplotted, the relations are extrapolated for SFGs with M_* < 10^9.5 M_⊙ and QGs with M_* < 10^10.3 M_⊙. The vertical dashed lines show the mass completeness limit of the CEERS field (gray) and Cosmic Vine (blue).