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Fig. 4

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Characteristic quantities q+ and u for all 57 considered cloud configurations under the assumption that the planetary signal can be separated from the stellar radiation (stellar radiation excluded) at an optimal wavelength of λ = 850 nm. The tuples of the characteristic quantities with equal total cloud coverages ctot are connected by solid lines and are represented by the same color. The tuples of the characteristic quantities with equal cap asymmetries σNS are connected by dashed lines. The error boxes indicate the uncertainties as expected for a polarimetric precision of ∆ p = 0.1%.

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