Probability of companion detection as a function of the distance to the star from pyMESS2. On the left, overview of the detection limit results based on radial velocity (≤ 5 au) and direct imaging (all SPHERE+NaCo observations, ≥5 au) data for the whole HD 95086 system. In the middle and right, direct imaging results are zoomed between 5 and 35 au. In the left and middle, coplanarity is assumed between the researched exoplanets and the outer belt (i.e., with i = −30 ± 3° and ω = 97 ± 3°), but not on the right. The results without the last five epochs imaged with SPHERE (in 2018 and 2019) are shown in gray to black contours for a given probability of 10%, 50%, 68%, 90%, and if coplanarity is assumed 99%. The color bars show the levels of probability detection.