Fig. 3

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Sky-projected obliquity λ (upper panels) and 3D obliquity ψ (bottom panels) as a function of the stellar effective temperature for the sample of planets around apparently single stars (left panels) and known binary or triple systems (right panels). Hot Jupiters (defined as having 0.4 < Mp/MJ < 13 and a/R⋆ < 11) are shown in red; warm Jupiters (0.4 < Mp/MJ < 13 and a/R⋆ > 11) are shown in orange; hot Saturns (0.2 < Mp/MJ < 0.4 and a/R⋆ < 11) are shown in green; and warm Saturns (0.2 < Mp/MJ < 0.4 and a/R⋆ > 11) are shown in blue. Systems with known binary WD companions are shown as stars. The Kraft break at ∼6100 K is shown as a dashed blue line. TOI-1259Ab is only one of the four WD systems with a measured true 3D obliquity.
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