Image Details
Caption: Figure 4.
Survey-averaged completeness to accreting companions as a function of projected separation (mas) and ﹩M\dot{M}﹩ (﹩{M}_{{\rm{J}}}^{2}\,{\mathrm{yr}}^{-1}﹩ ). The five GAPlanetS detections are overplotted as white stars. From upper left to lower right, these are CS Cha c, LkCa 15 b, HD 142527 B, PDS 70 c, and HD 100453 B.
© 2025. The Author(s). Published by the American Astronomical Society.