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Fig. 13


Companion mass and host star metallicity [Fe/H] for transiting brown dwarfs and low-mass stellar companions. We split the companions between 13–42.5, 42.5–80, and 80–150 MJup  to visualize possible metallicity differences between low-mass and high-mass brown dwarfs and low-mass stars. The histograms at the top display the number of companions in 0.1 dex [Fe/H] bins for these mass ranges.

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