Three different spectra of (55638) 2002 VE95 are reported in gray and the spectral models in black. The spectra are presented in the same order as in Fig. 1 (from the top to the bottom 2008, 2007, and 2006). Continuous and dashed dark lines represent the synthetic spectrum obtained with the Hapke model. Continuous and dashed parts represent, the ranges at which the model was computed and the ranges which are just completed respectively. Visible and near-infrared photometry were converted in reflectance (black filled circles with errors). The top two spectra were shifted by +0.2 and +0.4 unit for clarity.
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