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Fig. 1


a) Visible spectra of DA14 obtained with CAFOS (black) and OSIRIS (red). Filled circles are the reflectance R values. b) Same as the top panel, but adding the R values for the near-infrared. The mean spectrum of L-type asteroids from DeMeo et al. (2009) is shown in blue. Dashed lines indicate the variation range of this mean spectrum. Both the spectra and the reflectance R are normalized at the central wavelength of r′.

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