The high-albedo, low polarization disk around HD 114082 that harbors a Jupiter-sized transiting planet - Constraints from VLT/SPHERE completed with TESS, Gaia, and radial velocities

Open Access

Fig. 16

Sensitivity limits on bound companions, obtained by combining the constraints from IRDIS/IFS direct imaging, HARPS/FEROS RV and Gaia astrometry. The darkest area shows the parameter space where the probability of detecting a planet is less than 10%, while the white area corresponds to a probability higher than 99%.

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