Normalized cumulative distribution of orbital periods for planets with M_Psin(i) ≥ 0.8 M_Jup. The black line corresponds to the entire sample, while the blue and red line show the distribution for subsam-ples with M, < 1.4 M_⊙ and M_* ≥ 1.4 M_⊙, respectively. For comparison, the distribution for giant planets orbiting main-sequence stars with M_P sin(i) ≥ 0.8 M_Jup and P > 89 days is shown (obtained from the NASA Exoplanet Archive, selecting only planets discovered via RV and around host stars with log(ɡ) ≥ 4).