Fig. B.1

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Transit modelling of the wiggle in TESS Sector 22 based on the photometry as extracted from PDCSAP (left), SAP (mid), and PATHOS (right). The MCMCI analysis does not lead to any transit detection when attempting to fit a transit in the SAP and PATHOS photometry. The outcomes depend on the extraction pipeline, which plays against the genuineness of the putative transit event as confirmed by the BIC as well (see text for further details).
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