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Fig. 14

image

Granulation noise for three representative granulation stellar disk realizations of the Sun affecting the central part of the light curve for a terrestrial planet (Table 3). The colors denotes different wavelengths ranges (Table 2) in the optical (top panel) and in the near infrared (bottom panel). The relative difference is obtained subtracting, for each wavelength range, the light curve generated with the granulation snapshot with the one computed with the appropriate radially symmetric stellar limb darkened disk (see text).

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