Figure 6 from Global Climate and Atmospheric Composition of the Ultra-hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations

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Global Climate and Atmospheric Composition of the Ultra-hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations

Authors: Laura Kreidberg, Michael R. Line, Vivien Parmentier, Kevin B. Stevenson, Tom Louden, Mickäel Bonnefoy, Jacqueline K. Faherty, Gregory W. Henry, Michael H. Williamson, Keivan Stassun, Thomas G. Beatty, Jacob L. Bean, Jonathan J. Fortney, Adam P. Showman, Jean-Michel Désert, and Jacob Arcangeli

2018 The Astronomical Journal 156 17.

Provider: AAS Journals

Caption: Figure 6.

Phase-resolved planet-to-star flux ratios (points) compared to the best-fit blackbody (blue line) and the GCM with τ_drag4. Phases ϕ = 0.5 and 0.0 correspond to times of secondary eclipse and transit, when the substellar and antistellar points are respectively aimed at Earth. The blackbody model is fit to the HST/WFC3 data only. We also show a 100 ppm error bar in the lower right of each panel to emphasize the changing limits on the y-axes.

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