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Fig. A.1

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Phase-folded, and binned individual CHEOPS secondary eclipse observations of KELT-7b from visits 1 − 6, overplotted with the best-fitting CONAN3 model and arbitrarily shifted in flux for clarity. The left panel shows the nondetrended data overplotted with the full model, while the right panel shows the detrended data overplotted with the occultation model.

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