Fig. 1
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Detrended photometry from eight KELT-1b eclipses observed with CHEOPS centred around the eclipse centre time (Te). Each eclipse is observed as a single continuous CHEOPS visit of ≈7 h (labelled as V1-V8 in the figure), but the satellite’s orbital configuration leads to periodic gaps in the photometry, as described in Sect. 2.1.
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