Fig. 2
Spectra of (55638) 2002 VE95 in the visible as observed and their comparison. The first one from the top is the spectrum from 2004 (normalized at 0.55 microns) reported as a dotted line (shifted by +1.6 in reflectance for clarity), then the one of 2007, in a continuous line (shifted by +0.8 unit in reflectance for clarity) while the spectrum on the bottom with overimposed straight line is the division of the second spectrum by the first one and the linear fit performed to compute the mean slope variation. The surface observed in 2007 is redder than that observed in 2004.
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