Figure 2 from The Atmospheres of the Hot-Jupiters Kepler-5b and Kepler-6b Observed during Occultations with Warm-Spitzer and Kepler

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The Atmospheres of the Hot-Jupiters Kepler-5b and Kepler-6b Observed during Occultations with Warm-Spitzer and Kepler

Authors: Jean-Michel Désert, David Charbonneau, Jonathan J. Fortney, Nikku Madhusudhan, Heather A. Knutson, François Fressin, Drake Deming, William J. Borucki, Timothy M. Brown, Douglas Caldwell, Eric B. Ford, Ronald L. Gilliland, David W. Latham, Geoffrey W. Marcy, Sara Seager, and the Kepler Science Team

Désert et al. 2011 The Astrophysical Journal Supplement Series 197 11.

Provider: AAS Journals

Caption: Figure 2.

Phase-folded normalized Kepler occultation light curves. Plot for Kepler-5b is on top and Kepler-6b is on the bottom. The observations are the black points with their 1σ error bars. The data are binned by approximately 40 minutes (0.01 in phase). The best fits are overplotted with the red solid line.

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