Table 2
List of partial models derived from combined data sets.
| Asteroid | β | Δ | P | N lc | N app | N 689 | N 703 | ||
| [deg] | [deg] | [hours] | |||||||
|
|
|||||||||
| 391 | Ingeborg | −60 | 7 | 26.4145 | 24 | 2 | 141 | 96 | |
| 502 | Sigune | −44 | 3 | 10.92667 | 9 | 2 | 157 | 52 | |
| 616 | Elly | 67 | 23 | 5.29771 | 4 | 1 | 101 | 133 | |
| 1003 | Lilofee | 65 | 10 | 8.24991 | 107 | 83 | |||
| 1160 | Illyria | 47 | 23 | 4.10295 | 96 | 100 | |||
| 1192 | Prisma | −65 | 14 | 6.55836 | 5 | 1 | 44 | 43 | |
| 1276 | Ucclia | −49 | 22 | 4.90748 | 114 | 45 | |||
| 1307 | Cimmeria | 63 | 9 | 2.820723 | 2 | 1 | 91 | 54 | |
| 1339 | Desagneauxa | 65 | 17 | 9.37510 | 78 | 120 | |||
| 1396 | Outeniqua | 62 | 7 | 3.08175 | 2 | 1 | 112 | 68 | |
| 1493 | Sigrid | 78 | 7 | 43.179 | 78 | 103 | |||
| 1619 | Ueta | 39 | 6 | 2.717943 | 5 | 1 | 122 | 51 | |
| 1623 | Vivian | −75 | 8 | 20.5235 | 77 | 58 | |||
| 1738 | Oosterhoff | −72 | 8 | 4.44896 | 109 | 105 | |||
| 1838 | Ursa | 47 | 17 | 16.1635 | 102 | 91 | |||
| 2086 | Newell | −60 | 12 | 78.09 | 10 | 1 | 24 | 84 | |
| 3017 | Petrovic | −73 | 8 | 4.08037 | 3 | 1 | 114 | ||
| 3786 | Yamada | 56 | 2 | 4.03294 | 3 | 1 | 71 | ||
| 3896 | Pordenone | −32 | 9 | 4.00366 | 3 | 1 | 22 | 71 | |
| 4209 | Briggs | −56 | 25 | 12.2530 | 2 | 1 | 64 | ||
| 4467 | Kaidanovskij | 54 | 13 | 19.1454 | 20 | 107 | |||
| 6179 | Brett | −42 | 20 | 9.4063 | 6 | 1 | 93 | ||
| 7055 | 1989 KB | −61 | 11 | 4.16878 | 7 | 1 | 117 | ||
| 7360 | Moberg | −18 | 18 | 4.58533 | 3 | 1 | 103 | ||
Notes. For each asteroid, there is the mean ecliptic latitude β of the pole direction and its dispersion Δ. The other parameters have the same meaning as in Table 1. The uncertainty of the sidereal rotational period corresponds to the last decimal place of P.
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