Paper details measurements of the M-class asteroid and Rosetta flyby target 21 Lutetia from 2003-2008, investigating surficial variation in spectral properties. Data files show spectral comparison between different hydrated asteroids near 3 micrometers, using "type asteroids" for each main group that has been identified.
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themis_figure4.dat |
Two-column spectrum of 24 Themis from Figure 4. The first column is wavelength in micrometers, the second is reflectance normalized to 2.3 micrometers. |
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ceres_figure4.dat |
Two-column spectrum of 1 Ceres from Figure 4. The first column is wavelength in micrometers, the second is reflectance normalized to 2.3 micrometers. |
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pallas_figure4.dat |
Two-column spectrum of 2 Pallas from Figure 4. The first column is wavelength in micrometers, the second is reflectance normalized to 2.3 micrometers. |
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lutetia_figure4.dat |
Two-column spectrum of 21 Lutetia from Figure 4. The first column is wavelength in micrometers, the second is reflectance normalized to 2.3 micrometers. |
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lutetia_preprint.pdf |
Preprint of paper. |
