Open Access
Fig. 12.
Detection limits of 5σ for HiRISE derived in the present work for a bright nearby young star (H = 3.5, 19 pc, 20 Myr), compared to the 20% best SPHERE/SHINE detection limits. We overplot state-of-the-art population synthesis models based on the core accretion formation scenario (Mordasini 2018; Emsenhuber et al. 2020a,b).
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