Search completeness of the whole final combined sample (a), and of the AF (b), FK (c), and M (d) subsamples. This corresponds to the lower m_c sin i for which X% of the stars in the corresponding sample have detection limits below this m_c sin i at a given period P; from bottom to top: 40% to 90%. Our detected substellar companions HD 113337 b and HD 149790 B are shown as a red dot, while the nondetected planets of the SOPHIE survey, HD 128311 b and c, are shown as black dots (cf. Grandjean et al. 2021).