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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 2.

Hierarchical Bayesian inference of the ΔI distribution. The black curve shows the inferred distribution for the full sample, while the orange and blue curves correspond to systems hosting giant inner planets (Min > 0.3 MJup or 95 M) and lower-mass inner planets (Min < 0.3 MJup or 95 M), respectively. The gray dotted curve represents the isotropic expectation. The quoted ﹩{\rm{\Delta }}\mathrm{log}Z﹩ values are relative to the isotropic model.

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