Fig. 3
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The dayside (orange) and nightside (blue) planet-star flux ratio posterior distributions for all passbands. The central 68% posterior interval is marked with a dark shade and the previous dayside flux ratio estimates are shown as diamonds with errorbars showing their reported uncertainties. For TESS, the Beatty et al. (2020) estimate is shown on the left and the von Essen et al. (2021) estimate on the right.
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