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Fig. C.1

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Reflectance spectra of the asteroids from this work. Reflectance spectra from the SpeX instrument at the IRTF, Gaia DR3 and (when available SDSS are shown with grey stars, black filled circles and red filled circles, respectively. The green shaded areas represent the range of spectra for the A-types of the Bus-DeMeo taxonomy (DeMeo et al. 2009) for comparison to the observed reflectance spectra. The grey-shaded regions correspond to wavelength range of lower atmospheric transparency. Data in those regions, should be interpreted with care. Asteroids numbers from 254 to 3104 are shown here.

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