Observational constraints on f (number of 1–10 MJ planets per star) vs. orbital separation.
|Semimajor axes (AU)||Reference|
|0.07–0.33||0.008||Bonfils et al. (2013)|
|0.5–10.0||0.063 ± 0.0375||Cassan et al. (2012)|
|0–20||0.0625 ± 0.03||Montet et al. (2014)|
|10–100||<0.100 ± 0.001b||Bowler et al. (2015)|
|8–400||0.022||Lannier et al. (2016)|
Notes. (a) Assuming the planet mass function of Cassan et al. (2012). (b) For cold-start models, <0.154 ± 0.002.
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