Top: inferred orbital period and eccentricity for all systems with unimodal and bimodal posterior samplings from The Joker. Bottom left: inferred orbital period and surface gravity of the primary star, ﹩\mathrm{log}g﹩. The diagonal line indicates the orbital period of a hypothetical massless companion at the surface of a ﹩1.35\,{M}_{\odot }﹩ primary star with the given ﹩\mathrm{log}g﹩; the vertical line shows the same for ﹩\mathrm{log}g=0﹩, and the horizontal line shows the rough upper boundary of the red clump. Bottom right: stellar parameters for all primary stars in the unimodal and bimodal samples.