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Transiting Planetary Systems with Distant Giant Companions Remain Moderately Coplanar

  • Authors: Guang-Yao Xiao, 光耀 肖, Huan-Yu Teng, 环宇 滕, Xiumin Huang, 秀敏 黄, Fabo Feng, 发波 冯, Dong Lai, 东 赖, Fei Dai, 飞 戴, Yu-Juan Liu, 玉娟 刘

Guang-Yao Xiao et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure D1.

Forward Monte Carlo mapping between the Rayleigh width of the true mutual inclination (σψ) and that of the minimum mutual inclination (σΔI). The black curve is obtained from simulations with 105 systems, while the blue points show the median and 68% intervals from repeated realizations with N = 19, corresponding to the sample size of this work. The red dashed line marks the observed value, σΔI = 15﹩\mathop{.}\limits^{{\unicode{x000b0}}}﹩8.

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