Period vs. age plot for all giant exoplanets (0.2 R_J ≤ R_P ≤ 13 R_J) with well-constrained masses $\left({\sigma }_{M_{\text{P}}}/M_{\text{P}}\le 25\text{\%}\right)$ and radii $\left({\sigma }_{R_{\text{P}}}/R_{\text{P}}\le 8\%\right)$, periods of >10 days, and errors in age of σ_Age/Age ≤ 100%. TOI-4862 b is shown by the red star, illustrating its position as one of the youngest warm lupiters to date with a well-constrained age. The large age errors of most long-period giants are also evident.