Fig. 1

Illustration of the 586 asteroid spectra in the reduced VisNIR set. The vertical lines indicate the cutoff point between theB-DM and Gaia wavelengths. The red part of spectra is what remains in the Gaia wavelength range. The x-axes hold the wavelengths from 0.45 to 2.45 μm, while the y-axes are the reflectances normalized to unity at 0.55 μm.
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