Table 3
Summary of the results pertaining to our survey.
| Aster. | b / a | c / b | P sid | λ 1 | β 1 | λ 2 | β 2 | N dl | N opp | N 689 | N 703 | N LO | η a | D |
| [h] | [deg] | [deg] | [deg] | [deg] | [km] | |||||||||
|
|
||||||||||||||
| 122 | 0.85 | 0.96 | 10.6872 ± 1 | 30 ± 5 | 20 ± 10 | 209 ± 5 | 22 ± 10 | 24 | 6 | 181 | 108 | 0 | ( 70.7 ± 0.9 ) | |
| 172 | 0.93 | 0.90 | 27.4097 ± 4 | 171 ± 11 | −64 ± 10 | 14 ± 9 | −57 ± 10 | 61 | 6 | 159 | 75 | 0.17 | 77.4 ± 3.9 | |
| 236 | 0.88 | 0.86 | 12.3375 ± 1 | 196 ± 9 | 54 ± 10 | 36 ± 7 | 44 ± 10 | 57 | 5 | 187 | 120 | 0.16 | 86.0 ± 4.3 | |
| 387 | 0.93 | 0.88 | 24.14 ± 2 | 142 ± 8 | 51 ± 10 | 26 | 6 | 100.7 ± 5.3 | ||||||
| 402 | 0.88 | 0.70 | 10.6684 ± 1 | 306 ± 10 | −61 ± 10 | 162 ± 7 | −41 ± 10 | 15 | 4 | 169 | 65 | 0 | 64.6 ± 3.2 | |
| 458 | 0.86 | 0.80 | 21.81 ± 5 | 274 ± 6 | 33 ± 10 | 86 ± 5 | 14 ± 10 | 14 | 3 | 197 | 103 | 0.38 | ( 36.7 ± 0.4 ) | |
| 729 | 0.88 | 0.86 | 25.195 ± 1 | 88 ± 26 | −79 ± 10 | 60 | 3 | 182 | 104 | 0.14 | ( 50.0 ± 0.4 ) | |||
| 824 | 252.0 ± 7 | 25 | 2 | 133 | 149 | (32.5 ± 0.3) | ||||||||
| 980 | 0.93 | 0.83 | 20.114 ± 4 | 24.2 ± 6 | 35 ± 10 | 203 ± 5 | −5 ± 10 | 48 | 6 | 167 | 68 | 0.28 | ( 74.7 ± 0.6 ) | |
| 1332 | 32.120 ± 1 | 16 | 2 | 408 | (46.8 ± 0.1) | |||||||||
| 1372 | 15.23 ± 4 | 18 | 2 | 84 | 60 | ( 26.5 ± 0.3 ) | ||||||||
| 1702 | 21.15 ± 2 | 21 | 2 | 90 | 155 | ( 34.6 ± 0.1 ) | ||||||||
| 2085 | 111 ± 1 | 12 | 1 | 27 | 93 | ( 13.35 ± 0.04 ) | ||||||||
| 3844 | 13.33 ± 2 | 10 | 1 | 87 | (15.5 ± 0.7) | |||||||||
| 15552 | 33.63 ± 7 | 19 | 2 | 58 | ( 6.2 ± 0.2 ) | |||||||||
Notes. The b/a and c/b columns represent the relative axis dimensions of the ellipsoid best fitting the shape model. The Psid column indicates the sidereal rotation period of the asteroid in hours. The uncertainties are given with respect to the last digit. Columns λn and βn, with n = 1 and 2, represent the two or the unique pole solution(s). The Nx columns represent respectively the number of dense light-curves, the number of oppositions and the number of sparse points from the USNO (MPC code 689), Catalina (MPC code 703) and Lowell surveys. ηa represents the fraction of flat surfaces present on the shape model as inferred by the bootstrap method. Finally, the D column represents the equivalent diameter of the sphere having the same volume as the asteroid shape model. When we were not able to scale the shape model of the asteroid, the NEOWISE diameter Mainzer et al. (2016; or WISE diameter, Masiero et al. 2011, when NEOWISE data are unavailable) is given in parentheses.
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