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Fig. 4.

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Top: mass vs. orbital separation for companions with mass 1 ≤ Mc ≤ 20 MJup and a in the range 1 − 10 au orbiting stars with M < 0.75 M. Bottom: companion mass vs stellar mass. In both panels, black asterisks indicate objects detected by RV techniques, blue diamonds are companions identified in microlensing surveys, green triangles are companions uncovered via eclipse timing variations, and magenta pentagons correspond to objects with true masses determined by joint RV+astrometry analyses. The red hexagon indicates the location of GJ 463 b. Data are from https://exoplanetarchive.ipac.caltech.edu/.

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