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Fig. 4


Intensity profiles obtained from the cut at x = 0, y> 0 in the synthetic disk images of Fig. 2. The black curves are the overlap of N = 42 different images. The number N depends on the duration of the transit of Kepler 11-f (7 h, Table 3) and the observed granulation timescale for the Sun is ~10 min (see text). The intensity profiles are normalized to the intensity at the disk center (R = 0.0). The green line is the temporal average profile.

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