Notes. Sources listed in Table D.2 are not duplicated here. *Velocity dispersion only. **Local analogues. Lensed. The object is potentially a system undergoing a minor merger with mass ratios of ∼ 1 : 6 separated by ∼ 4 kpc (Cathey et al. 2024). Still, the low dispersion of the system ∼ 32 km s⁻¹ suggests the interaction has not significantly perturbed the dynamics. With an updated stellar mass of log(M_⋆/M_⊙) ≈ 10.39 and a log[SFR/(M_⊙ yr⁻¹)] ≈ 2.13, the galaxy would be shifted closer to the MS, with a revised ΔMS = 0.23 at z = 4.2.