A full transit of v2 Lupi d and the search for an exomoon in its Hill sphere with CHEOPS

Open Access

Fig. 4

Zoom on the detrended transit of v² Lup d from the middle panel of Fig. 2. Unbinned exposures are shown as sky blue points with error bars, and white points show a binning by a factor of 15 (or lower depending on how many exposures there are between two light-curve interruptions). The transit model is represented by an orange curve.

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