Fig. 11
Colour-magnitude diagrams considering the SPHERE H2-H3 (left panel), H2-K1 (middle panel), and K1-K2 (right panel) colours, comparing PDS 70b with the photometry of M, L, and T field dwarfs, young companions, and red dwarfs. The diagrams are overlaid with reddening vectors from interstellar extinction and 0.5 μm fosterite grains. See Chauvin et al. (2018) and Bonnefoy et al. (2018) for details about the CMDs.
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