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Fig. 8


Mass detection limits (90%) obtained combining all AU Mic DI data with MESS2 on the one hand (blue lines), and using MESS2 on RV data with the LPA approach on the other hand (red lines), for different orbital inclinations. The detection limits derived by MESS2 (multi-epoch DI and RV data combination) are represented by black lines. We use an eccentricity range of [0, 0.6], and Ngen = 10 000.

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