Figure 7 from Spin–Orbit Misalignment and Precession in the Kepler-13Ab Planetary System

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Spin–Orbit Misalignment and Precession in the Kepler-13Ab Planetary System

Authors: Miranda K. Herman, Ernst J. W. de Mooij, Chelsea X. Huang, and Ray Jayawardhana

2018 The Astronomical Journal 155 13.

Provider: AAS Journals

Caption: Figure 7.

Effect of contaminating light on fitted impact parameter. If the dilution is not accounted for, the best-fit model (based on the minimum ﹩{\chi }^{2}﹩) will have a larger impact parameter to compensate for the shallower transit depth. The black dots denote the minimum ﹩{\chi }^{2}﹩ values, indicative of the shift in impact parameter.

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