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Table 2

Taxonomic classification (both visual and using the M4AST online tool), as well as the computed spectral slopes for the observed asteroids.

Asteroid Visual M4AST - χ2 (10−3) Complex SVIS (10−5−1) SVNIR (10−5−1) Sample
61674 B Ch - 0.182 B - 0.342 C −1.7 ± 0.6 −0.2 ± 0.6 a
6671 Ch Cb - 0.191 Cgh - 0.274 C 1.4 ± 0.7 1.6 ± 0.5 c
5994 C Cgh - 0.192 C - 0.235 C 4.4 ± 0.3 −1.0 ± 0.7 b
23000 C/Cb Cgh - 0.077 C - 0.138 C 3.4 ± 0.8 1.6 ± 0.6 b
20094 X Xc - 0.169 X - 0.224 X 7.9 ± 2.0 0.9 ± 0.7 a
121281 X X - 0.242 Xc - 0.253 X 5.6 ± 0.8 0.9 ± 2.2 c
155547 Xk Xe - 0.100 Xk - 0.455 X 7.3 ± 1.0 1.3 ± 2.2 c
222080 C/X? O - 15.773 V - 17.429 X 2 ± 4 6.3 ± 1.3 a
198403 D? Cb - 31.374 X - 32.408 D 16.0 ± 0.3 40.3 ± 1.3 b
66648 S Sq - 0.448 Sr - 0.609 S 13 ± 6 −4.2 ± 1.4 a
20095 Sq Sq - 0.458 Sr - 0.654 S 5.4 ± 0.8 −9.0 ± 2.0 c
38466 S S - 0.353 Sv - 0.393 S 8.2 ± 0.8 −7.0 ± 2.0 c
22540 Sq B - 0.916 Cg - 1.166 S 3.7 ± 0.9 −8.3 ± 0.5 c
261489 - A - 21.854 L - 26.925 - 1 ± 4 8 ± 4 a

Ceres C C - 0.0096 Cb - 0.1087 C 1.2 ± 0.5 0.2 ± 0.9

Notes. The last column shows the sample to which asteroids belong (see main text for details).

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