Figure 7 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 7.

Dayside planet-to-star flux (points) compared to a blackbody model for the planet (dashed gray line) and the best-fit 1D model (blue line, with 1σ uncertainty shaded in orange) for the HST/WFC3 data (left) and Spitzer (right). The 1D model was fit to all the data simultaneously, but the blackbody was fit to the WFC3 data only. The best-fit 1D model binned at the resolution of the Spitzer data is indicated by blue squares (right).

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