Deviation from the FMR for high-z galaxies. We adopt the $\mu \equiv log(M_{\star }/{\mathrm{M}}_{\odot })-0.65log(\mathrm{SFR}/{\mathrm{M}}_{\odot }{\mathrm{yr}}^{-1})$ FMR obtained by Curti et al. (2020) for the high-sSFR galaxy subsample from the SDSS (z ≲ 2, York et al. 2000). We report the results of the weak feedback (ϵ_SN = 1/4), modulated accretion (A₁₀₀ = 1/3) models along with the data from JWST observations (Nakajima et al. 2023; Curti et al. 2024; Chemerynska et al. 2024b) and SERRA simulations (Pallottini et al. 2022).