Fig. 2
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Recovery fraction of injected transit signals similar to those of Hippke et al. (2019) injected into simulated PLATO stellar LCs of quiet (second column) and active (third column) stars, compared with the recovery fraction of similar signals injected into a sample of active stars observed by TESS (first column) and analyzed by H19. The biweight with a window of 1.0 day was not tested by H19 on TESS active LCs.
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