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Fig. 1


Detection probabilities when using all AU Mic DI data (top), all DI and RV data with our RMS approach (middle), and all DI and RV data with the LPA approach (bottom). We use a planet mass range of [0.5, 14] MJup, a separation range of [0.05, 20] au, an eccentricity range of [0, 0.6], an inclination range of [83°, 97°], and Ngen = 10 000.

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