Two different ways to visualize detectability within the survey. Detected planets (see Table 1) are plotted in black. Left: global detection efficiency of the combined survey in period-planet mass space. Planets with M_p sin(i) above the, e.g., 50% limit can be detected around 50% of the stars in the sample at the given period. Right: median detection probabilities of the combined survey in period-planet mass space (the 50% median probability curve is computed by determining the median of all individual stars’ 50% level at each period). Planets with M_p sin(i) above the 50% limit have a median detection probability of 50% across the sample at the given period.