Top: additional tests for host star mass. These additional tests are in good agreement with the similarities between the underlying eccentricity distributions of warm Jupiters orbiting higher-mass host stars with M_⋆ ≥ 1.15 M_⊙ and lower-mass host stars with M_⋆ < 1.15 M_⊙ seen in Figure 7. Bottom: additional tests run for planets orbiting at farther separations (100 days ≤ P < 365 days) and closer separations (10 days < P < 100 days) from their host stars. These tests reveal that the two underlying eccentricity distributions are in good agreement as seen in Figure 7 (see Figure 8 for additional details).