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Fig. 7

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Top panel: full absorption profiles for the PHNX (blue) and FTS (red) input spectra without active regions (solid lines), together with the corresponding profiles with a stellar spot (dashed lines). Bottom panel: differential signals obtained by subtracting the quiet-star profiles from the spot-crossing profiles. The color-coding matches the input spectra. The wavelength interval is the same as in Fig. 6.

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