Fig. B.1.

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Grouped by taxonomic class pseudo-reflectance spectra of asteroids based on two-color taxonomy. Top: g − r, i − z colors, middle: g − i, i − z colors, and bottom: r − i, i − z colors. We indicate the average wavelength of each filter in the lower plots. The distribution of values for each band is represented by whiskers (95% extrema, and the 25, 50, and 75% quartiles). For each, we also represent the associated template spectra of the Bus-DeMeo taxonomy (DeMeo et al. 2009).
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