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 Journal171.
Provider: AAS Journals
Caption: Figure 2.
Phase-folded TESS transit light curves of TOI-4495 b and c after accounting for TTVs, binned to 5 min. Red line is the best-fit photodynamics model (Section 5.3)