Kepler data analysis: non-Gaussian noise and Fourier Gaussian process analysis of star variability

2 Oct 2019Jakob RobnikUroš Seljak

We develop a statistical analysis model of Kepler star flux data in the presence of planet transits, non-Gaussian noise, and star variability. We first develop a model for Kepler noise probability distribution in the presence of outliers, which make the noise probability distribution non-Gaussian... (read more)

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