Fig. 2
Flux vs. wavelength for all the cases in Table 1. Solid lines plot the spectral distributions of the stellar unperturbed photospheres and dotted lines the spectral distributions of the star + spot systems with f0 = 0.5. In the top left we present the first case, in the top right the second case, in the bottom left the third case, and in the bottom right the fourth case.
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