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Fig. 1

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Mean reflectance of D-, T-, C-, Ch, and B-type asteroids normalised at 0.55 µm from the Bus-DeMeo taxonomy (DeMeo et al. 2009). We also include the P-type from the former Tholen taxonomy, which falls in the X-complex in DeMeo et al. (2009). Of the various sub-types in this complex (e.g. Xc, Xe, and Xk), we plot the mean reflectance of X-type asteroids (X_Mean) as a representative of the P-type. The shaded areas of top three curves denote the standard deviations of each taxon.

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