Gaia-predicted brown dwarf detection rates around FGK stars in astrometry, radial velocity, and photometric transits

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Fig. 7.

Histograms of the astrometric and radial velocity solid detections (Δχ² > 50) resulting from the P_distr = ‘Ma&Ge’ simulation. Top panel: host star magnitude. Second panel: period. Third panel: distance. Fourth panel: BD mass. Bottom panel: semi-major axis .

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