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Fig. 10


Examples of phase curves at different wavelengths (a: 0.465 μm; b: 0.550 μm; c: 0.749 μm; d: 0.900 μm) and different positions on the surface of Ceres as derived from OE data. Diamonds correspond to VIR observations and solid lines are fits obtained with Eq. (4). For each curve, the longitude and latitude of the corresponding position on the surface are indicated, along with the values of the fitted parameters. Curves are offset by 0.006 for clarity.

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