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TOI-4495: A Pair of Aligned, Near-resonant Sub-Neptunes That Likely Experienced Overstable Migration

  • Authors: Mu-Tian Wang, 王 牧天, Fei Dai, 戴 飞, Hui-Gen Liu, 刘 慧根, Kento Masuda, Andrew W. Howard, Samuel Halverson, Howard Isaacson, Elina Y. Zhang, Max Goldberg, Huan-Yu Teng, Ryan A. Rubenzahl, Benjamin Fulton, Erik A. Petigura, Steven Giacalone, Luke Handley, David W. Latham, Allyson Bieryla, Ashley Baker, Jerry Edelstein, Steven R. Gibson, Kodi Rider, Arpita Roy, Chris Smith, Josh Walawender, David Rapetti, Jon M. Jenkins, Joshua N. Winn

Mu-Tian Wang et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 5.

TTVs of TOI-4495 b and c. All observations are from TESS, except for the transit epoch of planet c near day 3100, which is from the KPF RM observation. The blue curves show TTV models from 50 random samples drawn from the photodynamical posteriors (Table 2), the red curve shows the best-fit solution, and the residuals are observed TTV minus the best-fit solution.

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