Figure 5 from Radial Velocity Observations and Light Curve Noise Modeling Confirm that Kepler-91b is a Giant Planet Orbiting a Giant Star

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Radial Velocity Observations and Light Curve Noise Modeling Confirm that Kepler-91b is a Giant Planet Orbiting a Giant Star

Authors: Thomas Barclay, Michael Endl, Daniel Huber, Daniel Foreman-Mackey, William D. Cochran, Phillip J. MacQueen, Jason F. Rowe, and Elisa V. Quintana

Barclay et al. 2015 The Astrophysical Journal 800 46.

Provider: AAS Journals

Caption: Figure 5.

Our marginal distribution on the model parameters R_p/R compared with Sliski & Kipping (2014). Our estimate has a much larger uncertainty. The estimate from this paper differs with the estimate of Sliski & Kipping (2014) by about 2.5 standard deviations.

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