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Fig. 22


SPHERE/IRDIS detection limits for the images in the K12 filter pair analyzed with TLOCI using ADI only for the systems PZ Tel (left) and HD 1160 (right). The mass limits are estimated from the atmospheric and evolutionary “hot-start” model BHAC15+COND (Baraffe et al. 2015). The relative magnitude of the companions and the mass predictions are derived for the K1 band.

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