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Table 5

List of improved asteroid models that were originally designated in DAMIT as “preliminary”.

Asteroid λ1 β1 λ2 β2 P Nlc Napp N689 N699 N703 NE12 NG96 N950 NHip
[deg] [deg] [deg] [deg] [h]
73 Klytia 266 68 44 83 8.28307 21 7 131 36 98 47
82 Alkmene 164 –28 349 –33 13.00079 11 1 158 72 36 38 192
132 Aethra 326 67 5.16827 4 2 204 55
152 Atala 347 46 199 61 6.24472 2 1 101 32
277 Elvira 121 –84 29.6922 22 5 142 36 51
278 Paulina 307 31 118 38 6.49387 3 1 195 51
311 Claudia 214 43 30 40 7.53138 23 6 114 33 108 40
484 Pittsburghia 70 46 10.64977 2 1 100 52
516 Amherstia 254 22 81 54 7.48431 5 3 162 32
534 Nassovia 66 41 252 42 9.46889 16 6 151 64 32
614 Pia 348 48 162 27 4.57872 2 1 121 78
714 Ulula 224 –10 41 –5 6.99837 9 2 177 67
770 Bali 70 50 262 45 5.81894 2 1 131 52
915 Cosette 350 56 189 61 4.469742 1 1 106 32 35
1012 Sarema 45 67 253 63 10.30708 2 1 74 42
1022 Olympiada 46 10 242 52 3.83359 5 2 107 91
1088 Mitaka 280 –71 3.035378 1 1 104 39 41
1223 Neckar 252 28 69 30 7.82401 16 7 132 33 60 36

Notes. Pole solutions preferred by asteroid occultation measurements (Ďurech et al. 2011) are emphasized by a bold font.

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