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Kepler-1624b Has No Significant Transit Timing Variations

  • Authors: Haedam Im, Morgan Saidel, Heather A. Knutson, Michael Greklek-McKeon, Shreyas Vissapragada, Karen A. Collins, Akihiko Fukui, Norio Narita, Kimberly Paragas, Richard P. Schwarz, Avi Shporer, Gregor Srdoc

Haedam Im et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 2.

Kepler light curve before detrending (left) and after detrending (right). The red line shows the Gaussian kernel convolution trend described in Section 2.2. Blue points indicate masked data (±0.8 transit durations around each transit midtime).

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