The Eccentricity Distribution of Short-period Planet Candidates Detected by Kepler in Occultation
@article{Shabram2016TheED, title={The Eccentricity Distribution of Short-period Planet Candidates Detected by Kepler in Occultation}, author={M. Shabram and B. Demory and J. Cisewski and E. Ford and L. Rogers}, journal={The Astrophysical Journal}, year={2016}, volume={820}, pages={93} }
We characterize the eccentricity distribution of a sample of ~50 short-period planet candidates using transit and occultation measurements from NASA's Kepler Mission. First, we evaluate the sensitivity of our hierarchical Bayesian modeling and test its robustness to model misspecification using simulated data. When analyzing actual data assuming a Rayleigh distribution for eccentricity, we find that the posterior mode for the dispersion parameter is σ =0.081 ± _(0.003)^(0.014). We find that a… CONTINUE READING
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