Posterior mean SFHs derived for the COSMOS-Web galaxies via SED modeling. Galaxies are classified based on their migration angle (Φ_Δt) over the last 500 Myr. Galaxies with Φ_Δt between −90° and −60° exhibit fast-declining SFH, while those with Φ_Δt ranging from −60° to −10° show slow decline. Star-forming galaxies with relatively recent flattening of their SFH fall within Φ_Δt between −10° and 60°. In contrast, those with constantly rising recent SFH are categorized with Φ_Δt between 60° and 90°. These classifications highlight diverse evolutionary trajectories among galaxies. The red and black lines correspond to selected galaxies with higher and lower migration vector norms to the median values (r₅₀₀ = 2 dex/Gyr), respectively. Shaded regions present the confidence intervals.