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

Open Access

Fig. D.2

Example result of the fitting method described in Sect. D with one transit (N = 1). Top: DRP fluxes for the visit of v² Lup d. Middle upper: Linear model of the instrumental vectors and the components of the PSF PCA, Middle lower: N = 1 transit model. Bottom: Residuals to linear model plus N = 1 transit model.

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