Fig. 1.

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Comparison of different reduced TESS light curves of HD 112429. Top: custom reduced short-cadence light curve, illustrated for sectors 14 and 15. The gaps in the light curve are caused by the data downlinks of TESS. Middle: absolute differences between our custom reduced light curve and the FFI lightcurve (blue), TESS-SPOC SAP flux (red) and PDC-SAP flux (black). Bottom: zoom-in of absolute differences between our custom reduced light curve and the FFI lightcurve (blue) and TESS-SPOC SAP flux (red).
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