Mass ratio vs. stellar mass for confirmed giant planets and brown dwarf companions (1 M_Jup <  M <  80 M_Jup) to late M-type and massive brown dwarf primaries (0.03 M_⊙ <  M <  0.3 M_⊙). Masses of RV companions actually correspond to Msini. Detection methods are labeled with different colors; the semimajor axes or, if not available, projected separations have been grouped in four bins, with each one being associated with a circle size. The position of HIP 81208, provided with errorbars, is explicitly labeled.