Fig. 7

In dark blue, the observed mass spectrum from the WASP planet survey and the EBLM binaries released in this paper. The orange histogram depicts the results from Grether & Lineweaver (2006), normalised to the number of WASP and EBLM objects heavier than 1 MJup. The vertical grey lines denote the rough mass limits for deuterium burning (13 MJup) and hydrogen burning (80 MJup). There is an evident deficit of objects between these two limits, which corresponds to the realm of brown dwarfs.
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