Fig. 4

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Absolute CMDs in the optical and near-IR for all the sources in the sample. Colored circles and diamonds with error bars represent the A and B components, respectively, for each pair for which the parallax difference is consistent within parallax errors, while gray error bars represent systems with discrepant parallaxes. In all panels, dashed lines represent the Baraffe et al. (2015) isochrones. In the right-most panel, the solid and dot-dashed lines represent the cloudy and clear atmosphere models of Saumon & Marley (2008), respectively. The three marks at 3, 10, and 20 Myr represent the limit of 13 MJup for the associated isochrones.
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