Fig. 1

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Comparison between the deconvolved images of (65) Cybele (top row) and the corresponding synthetic images generated by the OASIS tool (Jorda et al. 2010) of the ADAM, MPCD, and SAGE shape models. The red arrows indicate the direction of the spin axis. Observing conditions for the images are listed in Appendix A. Residuals between the observed and synthetic images are shown in Appendix D.
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