Table 8
Fraction of stars with cold Jupiters in our sample compared with those from previous works.
| Planetary mass [MJup] | Orbital separation [AU] | fCJ|SP[%] from Keplerians | fCJ|SP[%] from Keplerians and trends | fCJ[%] (Wittenmyer et al. 2020) | fCJ|SP[%] (1) (Bryan et al. 2019) |
|---|---|---|---|---|---|
| 0.3–13 | 1–2 |  |
− |  |
– |
| 0.3–13 | 2–4 |  |
− |  |
– |
| 0.3–13 | 4–10 | < 3.8 | − |  |
– |
| 0.3–13 | 1–10 |  |
 |
 |
– |
| 0.5–13 | 1–10 |  |
 |
– |  |
| 0.5–13 | 1–20 |  |
 |
– |  |
| 0.5–20 | 1–10 |  |
 |
– | 38 ± 7 |
| 0.5–20 | 1–20 |  |
 |
– | 39 ± 7 |
Notes. From left to right, the columns report the intervals of planetary mass and semi-major axis; the fraction of stars with cold Jupiters (fCJ|SP) in our sample by considering Keplerian signals only (third column) as well as including the long-term trend of K2-12 (fourth column), because it is still compatible with a planetary companion; the occurrence rates of cold Jupiters derived by Wittenmyer et al. (2020) and Bryan et al. (2019). (1)fCJ|SP for 1 < Mp < 10 M⊕ instead of the wider range 1 < Mp < 20 M⊕ used in both this work and Zhu & Wu (2018).
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