Open Access

Fig. 15


Search completeness of our combined survey. From bottom to top: 0 to 100% search completeness (i.e. the fraction of stars with good enough detection limits to rule out a companion of a given mp sin i at a given orbital period P). Black dots: confirmed GPs detected in the combined survey. HD 16232b, whose detection was confirmed by Kane et al. (2015), is included here (see Sect. 3.1.2).

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