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TTV-determined Masses for Warm Jupiters and Their Close Planetary Companions

  • Authors: Dong-Hong Wu, Songhu Wang, Ji-Lin Zhou, Jason H. Steffen, and Gregory Laughlin

2018 The Astronomical Journal 156 96.

  • Provider: AAS Journals

Caption: Figure 5.

Transit timing variations (blue dots) of the planets in Kepler-117 compared to our best fit (connected open yellow–green circles) obtained using the full Kepler data set. The residuals of TTVs for each planet are shown as green dots below the corresponding panels.

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