Removing biases on the density of sub-Neptunes characterised via transit timing variations - Update on the mass-radius relationship of 34 Kepler planets

Open Access

Fig. 4

TTVs of the near-resonant pair Kepler-128 b,c. Black bars show the pre-extracted transit timings from Rowe et al. (2015), while blue bars show the best photodynamical fit. Dashed red and green curves show sinusoidal approximations for the pre-extracted transits and the photo-dynamical analysis respectively.

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