Table 4
GP occurrence rate around AF dwarf stars.
mpsini | Orbital period | Search | Detected | Missed | GP occurrence rate | Confidence intervals | |
interval | interval | completeness | GP systems | GP systems | (%) | 1σ | 2σ |
(MJup) | (day) | C (%) | (%) | (%) | |||
|
|||||||
13–80 | 1–10 | 98 | 0 (<1) | ≤0.02 | ≤1 | 0–3.8 | 0–6.9 |
(BD) | 96 | 0 ( < 1) | ≤ 0.04 | ≤ 2.3 | 0–8.2 | 0–14.4 | |
100 | 0 ( < 1) | 0 | ≤ 1.9 | 0–6.8 | 0–12.1 | ||
|
|||||||
1–100 | 95 | 0 (<1) | ≤0.05 | ≤1.1 | 0–4 | 0–7.2 | |
91 | 0 ( < 1) | ≤ 0.1 | ≤ 2.5 | 0–8.6 | 0–15.2 | ||
98 | 0 ( < 1) | ≤ 0.02 | ≤ 1.9 | 0–6.9 | 0–12.3 | ||
|
|||||||
1–1000 | 91 | 0 (<1) | ≤0.1 | ≤1.1 | 0-4.1 | 0–7.5 | |
85 | 0 ( < 1) | ≤ 0.18 | ≤ 2.6 | 0–9.3 | 0–16.3 | ||
97 | 0 ( < 1) | ≤ 0.03 | ≤ 2 | 0–7 | 0–12.4 | ||
|
|||||||
1–13 | 1–10 | 86 | 0 (<1) | ≤0.16 | ≤1.2 | 0–4.4 | 0–7.9 |
(“Jupiters”) | 75 | 0 ( < 1) | ≤ 0.33 | ≤ 3 | 0–10.5 | 0–18.4 | |
96 | 0 ( < 1) | ≤ 0.04 | ≤ 2 | 0–7.1 | 0–12.5 | ||
|
|||||||
1–100 | 77 | 0 (<1) | ≤0.3 | ≤1.3 | 0–4.9 | 0–8.8 | |
57 | 0 ( < 1) | ≤ 0.76 | ≤ 3.9 | 0–13.8 | 0–24.3 | ||
95 | 0 ( < 1) | ≤ 0.05 | ≤ 2 | 0–7.2 | 0–12.7 | ||
|
|||||||
1–1000 | 64 | 2 | 1.1 | 3 | 2.4–7.7 | 1.3-12.6 | |
35 | 0 ( < 1) | ≤ 1.82 | ≤ 6.3 | 0–22.2 | 0–38.9 | ||
90 | 2 | 0.22 | 4 | 3.1–9.9 | 1.7–16 | ||
|
|||||||
0.3–1 (“Saturns”) | 1–10 | 83 | 0 ( < 1) | ≤ 0.2 | ≤ 2.3 | 0–8.2 | 0-14.5 |
|
|||||||
1–100 | 63 | 0 ( < 1) | ≤ 0.58 | ≤ 3 | 0–10.8 | 0–19.1 | |
|
|||||||
1–1000 | 48 | 0 ( < 1) | ≤ 1.1 | ≤ 3.9 | 0–14 | 0–24.9 |
Notes. The parameters are displayed in normal, bold or italic fonts when considering the full star sample, the most massive (M⋆> 1.5 M⊙) stars only or the least massive (M⋆≤ 1.5 M⊙) stars only, respectively. For mpsini in the 0.3 to 1-MJup range, we display the GP occurrence rate and other parameters only for our low-M⋆ sub-sample, as our completeness is almost null in this domain for our higher-mass targets.
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