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Table 2

Constraints on the frequency of substellar companions.

Mass range s.m.a. range Evol. model Ages SpT Planet model Median 68% CI
[MJup] [au] [%] [%]
Parametric model

1–75 5–300 BEX-COND-hot Nominal BA Full 23.0 13.3–36.5
BDB 4.1 1.1–8.3
PPL/LN 14.8 6.9–28.6

1–75 5–300 BEX-COND-hot Nominal FGK Full 5.8 3.0–10.5
BDB 3.2 1.4–6.2
PPL/LN 0.4 0.0–4.0

1–75 5–300 BEX-COND-hot Nominal M Full 12.6 5.5–25.5
BDB 5.4 1.0–14.1
PPL/LN <9.7

Parametric model – impact of input assumptions

1–75 5–300 BEX-COND-hot Nominal FGK Full 5.8 3.0–10.5
Minimum 5.7 3.0–10.1
Maximum 6.0 3.1–10.8
1–75 5–300 BEX-COND-warm Nominal FGK Full 5.9 3.1–10.6
1–75 5–300 COND-2003 Nominal FGK Full 6.0 3.1–10.7
1–75 10–300 BEX-COND-hot Nominal FGK Full 5.5 2.8–9.5

Synthetic population model

1–75 5–300 BEX-COND-hot Nominal FGK Full 5.7 2.9–9.5
GI 1.5 0.5–3.6
CA 2.5 0.8–5.6

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