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Table 1

Distribution of observations and asteroids over taxonomic classes and orbital populations.

Fraction Orbital Class
Class Samples Asteroids This work DM09 NEA MC H IMB MMB OMB Cyb Hilda JT
A 57 32 1.5 1.6 2 3 2 7 10 8
B 68 45 2.1 1.1 15 4 1 12 5 8
C 299 221 10.4 7.3 69 8 2 89 72 79 2 2 5
Ch 144 107 5.0 4.8 9 2 20 47 26 2 1
D 119 82 3.9 4.3 6 1 1 4 5 5 16 44
E 65 46 2.2 7 4 27 4 3 1
K 59 42 2.0 4.3 21 2 5 2 12
L 76 58 2.7 5.9 20 4 3 4 22 3 2
M 252 142 6.7 29 7 2 17 47 28 2 10
O 4 2 0.1 0.3 1 1
P 195 135 6.4 14 6 1 11 26 36 12 12 17
Q 158 107 5.0 2.2 89 5 7 4 2
R 15 10 0.5 0.3 7 2 1
S 1188 898 42.3 53.8 404 101 35 140 172 45 1
V 206 142 6.7 4.6 28 2 104 4 4
X 50 33 1.6 8.6 20 8 2 1 2
Z 28 23 1.1 1 1 4 6 3 1 7
Σ 2983 2125 100 98.9 741 157 76 428 425 264 21 34 86

Notes. The second column gives the number of observations assigned to each class, while the third and all following columns refer to the number of individual asteroids assigned to the class. DM09 refers to DeMeo et al. (2009). The fractions in this column do not add up to 100%, due to the missing T-class in this scheme. The orbital classes use the following acronyms: NEA – near-Earth asteroids; MC – Mars-crosser; H – Hungaria; IMB – inner main belt; MMB – middle main belt; OMB – outer main belt; Cyb – Cybele; JT – Jovian trojans.

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