Simulations of starspot anomalies within TESS exoplanetary transit light curves - I. Detection limits of starspot anomalies in TESS light curves

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Fig. 11

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Plot of ΔF_p and ΔF_spot calculated from Eq. (4) and (7) combined with the best fitting model (solid black line). The blue data points represent the M4V host star results. The red data points represent the M1V host star results, while the green data points represent the K5V host star results.

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