Delay in mean mass assembly look-back times caused by environment (Δ_env). The results using T₅₀, T₇₀, and T₉₀ appear in the first, second, and third panels, reading from top to bottom. We consider galaxies of low (10⁹ − 10¹⁰ M_⊙) and high masses (10¹⁰ − 10¹¹ M_⊙) on the left and right panels. Every column corresponds to a Δ_env value, where C, F, and V depict clusters, filaments, and voids respectively, aiming to compare every LSS environment. Also, Δ_local corresponds to the difference between groups and singlets. Rows in every panel depict SFH types (short-timescale SFH, long-timescale SFH, or both altogether).