Radial velocity of HD 209458 b (dashed line). The shaded area indicates the timespan of the observations. The inset shows the different observations with the vertical line indicating the end of the secondary eclipse with the ephemeris value from Knutson et al. (2007) and the corresponding transit duration from Beaulieu et al. (2010). Only observations after this point contain the combined light of the planet and host star.
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