Fig. 5

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Average detection probability of a companion of given mass/sma in the BEAST intermediary survey using the cond atmospheric model. The two detected planets in this survey are also represented with the mass/sma extracted from Janson et al. (2021a) and Squicciarini et al. (2021). Jupiter is also added to provide a comparison. In the case of b Centauri b, no semi-major axis estimation is available, so we provide its projected separation instead.
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