Fig. 6
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Distribution of stellar obliquities for hot and warm Jupiters from our ELK simulations (blue histogram), compared to the measured obliquity of TOI 1259Ab including 1σ uncertainties (gray-shaded region). About 14% of the simulated close-in Jupiter systems have final obliquities consistent with the measured obliquity (19% if any systems with obliquities lower than our measurement are included).
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