Fig. 4

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phase curves of five hot Jupiters after CBV detrending and removing the Gaussian process, which captures stellar and instrumental artifacts. The four components of the phase curve are: reflected light (blue), thermal emission (orange), ellipsoidal variations (green), and Doppler beaming (dark red), along with the composite model in thick red. The unbinned 30-min Kepler time series is shown in gray circles and is used in the fit, and median-binned photometry is shown with black circles for ease of visualization.
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