Sky-projected obliquity (∣λ∣) as a function of stellar age for systems younger than 1 Gyr. Systems with well-constrained ages (fractional uncertainty ≤ 30%) are shown in purple, while those with poorly constrained ages (>30%) are shown in gray. Planets with radii R_p < 6 R_⊕ or masses M_p < 30 M_⊕ are highlighted with red-edged markers and labeled individually. The Kozai–Lidov and secular-interaction contours are adapted from G. Zhou et al. (2020), where Kozai interactions can occur over 10⁴–10⁸ yr and secular interactions may take over hundreds of megayears. The blue-shaded region highlights the regime in which tidal evolution is expected to become important. Giant planets with strong misalignment (∣λ∣ > 50°) are also labeled. Our targets, TOI-560 b (yellow) and TOI-5082 b (green), are highlighted for comparison.