Detection probability as function of companion mass and semi-major axis. The contour plots have been calculated using the AMES-COND and AMES-DUSTY evolutionary models, relying on the contrast curves generated for the 53 targets of the SHARDDS survey (Fomalhaut C and HD 107649 have been rejected due to respectively adverse observing conditions and the presence of extended bright structures). The estimated mass and semi-major axis estimated for 21 targets of the SHARDDS survey by Pearce et al. (2022) are injected in the probability map along with the associated uncertainties.