Fig. 1
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Color-magnitude diagram showing the position of HR 2562 B (red hexagon, Konopacky et al. 2016) relative to the population of low-mass stars and brown dwarfs (colored circles), as obtained from Best et al. (2020). The different colors highlight the different spectral types. The gray pentagons correspond to selected directly imaged planets (DIP) and planetary-mass companions (PMCs).
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