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Fig. 23


SPHERE/IFS detection limits for the YJH spectral data cubes analyzed with PCA using ADI only for the systems PZ Tel (left) and HD 1160 (right). The resulting spectral data cube was collapsed before the estimation of the detection limits. The mass limits are estimated from the atmospheric and evolutionary “hot-start” model BHAC15+COND (Baraffe et al. 2015). The plotted relative magnitude of the companions is in the J band and the mass derived from model predictions in this band.

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