Combined results from SEGUE, APOGEE, and LAMOST surveys. The main panels show the line-of-sight velocity relative to Λ_⊙ for the Sgr Stream across four metallicity bins. Background gray, orange, and green scatter points represent particles from the V21 simulation classified as still-bound, young wrap (0 > T_s ≥ −2 Gyr), and old wrap (T_s < −2 Gyr), respectively. Overlaid symbols show observed Sgr Stream members: circles for SEGUE, triangles for APOGEE, and diamonds for LAMOST. Red symbols indicate stars with T_s ≥ −2 Gyr, while blue symbols indicate T_s < −2 Gyr. The left panels display stripping time distributions for observed stars within each metallicity bin. The figure demonstrates that as metallicity decreases, the fraction of young wraps decreases while old wraps increase.