Cold Jupiters and small planets: Friends, foes, or indifferent? - A search for correlations with the largest exoplanet samples

Open Access

Fig. C.2

Similarly to Fig. 1, occurrence rates of CJs with M_p = 0.5–20 M_Jup in the AAT (orange), CLS (violet), and HARPS (green) RV surveys, at sub-solar ([Fe/H] < –0.1), solar (–0.1 ≤ [Fe/H] ≤ 0.1), and super-solar ([Fe/H] > 0.1) metallicity. Almost identical occurrence rates are obtained for M_p = 0.3–13 M_Jup. See Table F.2.

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