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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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