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Fig. 6


Simulation of the combination of two DI observations. The second DI data are assumed to be obtained 5 (left) and 25 yr (right) later. 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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