The λ distributions for hot-Jupiter (3 × 10⁻⁴ ≤ m_p/M_⋆ ≤2 × 10⁻³, a/R_⋆<10), sub-Saturn (3 × 10⁻⁵ ≤ m_p/M_⋆ ≤3 × 10⁻³), warm-Jupiter (3 × 10⁻⁴ ≤ m_p/M_⋆ ≤2 × 10⁻³, a/R_⋆>11), compact multiplanet (period ratio of adjacent planets, P_i+1/P_i < 6), massive-planet systems (2 × 10⁻³ ≤ m_p/M_⋆), and eccentric Jupiters (3 × 10⁻⁴ ≤ m_p/M_⋆ ≤2 × 10⁻³, e > 0.1), along with the Kraft break and its associated uncertainty derived in this work. In terms of T_eff coverage, only the hot-Jupiter systems have sufficient measurements (>10) in the hot-star regime. Sub-Saturns with nearby companions are marked in blue. The predicted relation between T_eff and λ from secular resonance crossing (C. Petrovich et al. 2020; E. Dugan et al. 2025) is shown as the light-blue shaded region.