Fig. 6
Configuration of HD 189733 and the modeled variations of the flux and polarization (q,u, and p) at 4500 Å. The planet is orbiting from the bottom to the top in front of the star. Solid and dash-dotted lines represent the calculations for the PPM and SphM atmospheres for the host star, respectively. The dashed line in the top left panel defines the planetary orbit behind the star.
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