Fig. 11

Absorption profiles in the Mg i line calculated with the fluxes averaged over transit and post-transit observations of HD 209458b. The observed profile (Vidal-Madjar et al. 2013) is displayed as a blue histogram with a resolution of 20 km s-1, while the solid black line corresponds to the theoretical global best-fit profile. The associated with this absorption profile is 225.9 (357 data points), and the χ2 for all observations is 802.4 for 1067 degrees of freedom.
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