Fig. 10
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Transmission LCs of HD 209458b in comparison with models of the CLV+RM effect from synthetic stellar spectra, colored as in the figure legend. Left: transmission LC computed in a passband of 0.75 Å around the Na I D lines, averaged together, and binned to 0.001 in orbital phases for better visualization. Right: transmission LC in a passband of 0.4 Å. In the bottom panels, we show the difference between the binned data and the models.
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