Fig. 11
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Sodium doublet of KELT-11 b with two best fits retrieved with MERC overlaid. In gray, the original data in absorption, in black, the data binned by ×5 for better visibility. In orange the best fit applying the basic model with no winds, only planetary rotation is shown, in blue the overall best fit is shown, for the model with a day-to-night side wind at approximately 5 km s−1.
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