Fig. 1

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Comparison between the VLT/SPHERE/ZIMPOL deconvolved images of Kleopatra and the corresponding projections of our MPCD and ADAM shape models. The red arrow indicates the orientation of the spin axis. We used a realistic illumination to highlight the local topography of the model using the OASIS software (Jorda et al. 2010). The residuals of both models are shown in the two bottom rows, more specifically those are chi-square pixel residuals in units of the instrumental noise associated to each pixel (photon and readout noise).
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