SIMBAD references

Our understanding of the occurrence rates and demographics of long-period planets depends critically on data from legacy radial-velocity surveys with the long-term sensitivity to Jupiter-like planets in Jupiter-like orbits. A recent paper presented such an analysis for giant planets (m sin i > 0.3 M_J) from the now-completed Anglo-Australian Planet Search. In this work, I deliver the detailed detection sensitivities for all 203 individual stars in that study, as a function of orbital periods from 100 to 6000 days. We present these data as a companion to Wittenmyer et al.