Fig. B.2
Comparison of non-rectified light curves for fading effects of the Be star CoRoT 102719279 (star No 9) observed during the IR1, LRA1, and LRA6 runs. The light curves are arbitrarily displaced in the ordinates, while their right flux levels are shown in Fig. B.1. The same sampling is used for all light curves (S1). The time in the abscissas indicates only the duration of the respective runs.
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