Fig. 3
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Detection probability of point sources as a function of the semi-major axis of point sources for Vega, using a combination of the 2018 NIRC2 observation and the TRES radial velocity measurements from Hurt et al. (2021) (see Sect. 3.1.2). We can reach an ~8 MJupiter detection limit at ~4 au, while probing down to ~2–~3 MJupiter at 0.1 au and 22 au, respectively.
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