Fig. D.1
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HD 20329 TESS photometry and TLCM fit. Left panel: TESS normalized SAP-fluxes vs time. Black dots are the observations. The red curve is the result of the simultaneous transit + occultation + beaming + reflection + ellipsoidal + wavelet-based noise model fit. Top right panel: Primary transit of HD 20329b (black dots) and best model fit (red line) after subtracting the red-noise component from the light curve (top). Bottom right panel: Residuals of the fit.
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