Image Details
Caption: Figure 6.
Projected stellar obliquity vs. estimated stellar age for all hot/warm Jupiters. Planets are colored by a/R⋆ and labeled in triangles or circles given their host star effective temperatures (i.e., triangles for host stars above the Kraft break Teff > 6250K and circles for stars below the Kraft break). Gray lines show 1σ uncertainties. For TOI-1268, we plot its estimated age between the 120 Myr Pleiades and 670 Myr Praesepe clusters and its stellar obliquity using representative values inferred from SERVAL RVs labeled in blue error bars. The 3σ credible interval of obliquity posteriors derived from the RV and DT signals are shown in black.
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© 2022. The Author(s). Published by the American Astronomical Society.
