Distribution of debris disks detected by SPHERE in the separation a – mass plane (red open squares). For comparison, the distributions of stellar and planetary companions is also shown (see Tables H.1 and H.2). White triangles are companions detected using RV; orange filled circles are companions detected in DI; green filled squares are companions whose presence is deduced from astrometric perturbation. The masses of the debris disks have been multiplied by 100 to reduce the size of the plot. The gray background gives the number of program stars where the search of debris disks by SPHERE is sensitive (see scale on bottom of the figure).