Figure 1 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 1.

Photometric time series we used in the analysis in this work is shown in gray. The light curve has been normalized to zero median. In blue we show the radial velocity data we collected using the Hobby–Eberly Telescope. The photometric and RV data are on the same time axis.

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