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Table 3

List of new asteroid models derived from combined data sets or sparse data alone.

Asteroid λ1 β1 λ2 β2 P Nlc Napp N689 N699 N703 NE12 NG96 N950 NHip
[deg] [deg] [deg] [deg] [h]
10 Hygiea 312 –42 122 –44 27.6591 23 9 263 405 50
13 Egeria 44 21 238 11 7.04667 13 4 255 74 203 34
14 Irene 97 –22 268 –24 15.02991 20 8 250 48 161 45
37 Fides 270 19 89 27 7.33253 23 5 270 61 135 31
40 Harmonia 22 31 206 39 8.90848 19 6 210 48 255 102
42 Isis 106 40 302 28 13.58364 28 7 210 36 128 51
62 Erato 87 22 269 23 9.21819 1 1 164 48
68 Leto 103 43 290 23 14.84547 12 2 174 85 30 152
69 Hesperia 250 17 71 –2 5.65534 35 7 222 44 40
97 Klotho –1 30 161 40 35.2510 25 6 309 31 202
119 Althaea 339 –67 181 –61 11.46514 4 2 149 59 222
162 Laurentia 139 64 313 51 11.86917 4 2 166 31 40
174 Phaedra 94 36 266 14 5.75025 2 1 173 36
188 Menippe 32 48 198 25 11.9765 4 1 145 40
258 Tyche 224 –4 40 –9 10.04008 10 2 162 44
264 Libussa 157 18 338 –9 9.22794 19 3 129 39 49
291 Alice 69 51 249 56 4.316011 9 4 75 46
302 Clarissa 28 –72 190 –72 14.47670 8 2 102 104
310 Margarita 225 –35 42 –33 12.0710 27 1 88 31 51
312 Pierretta 82 –39 256 –58 10.20764 4 1 176 36 52
336 Lacadiera 194 39 37 54 13.69552 3 1 121 36 32
340 Eduarda 188 –43 18 –47 8.00613 2 1 117 76 31 36
354 Eleonora 144 54 4.277186 37 9 258 40 139 96
355 Gabriella 341 78 197 70 4.82899 4 1 128
367 Amicitia 203 38 21 32 5.05502 2 1 128 34
372 Palma 221 –47 44 17 8.58189 28 6 214 52 36
376 Geometria 239 45 63 53 7.71097 39 9 158 76
399 Persephone 36 63 9.14639 166 36
400 Ducrosa 328 56 158 62 6.86788 3 1 103
413 Edburga 202 –45 15.7715 2 1 148 43
436 Patricia 124 –30 339 –58 16.1320 4 1 97 53 91
440 Theodora 80 –88 4.83658 123 103 48
471 Papagena 223 67 22 18 7.11539 13 2 293 72 203 112
486 Cremona 227 59 31 30 65.151 1 1 127 55 35
499 Venusia 37 50 212 46 13.4871 4 1 122 39 31
544 Jetta 275 –84 31 –67 7.74528 3 1 139 60
573 Recha 74 –24 252 –48 7.16586 3 1 161 85
584 Semiramis 106 –56 315 –32 5.06893 24 6 150 59 49
590 Tomyris 273 –47 120 –46 5.55248 3 1 91 32
601 Nerthus 173 44 20 32 13.5899 139 94
606 Brangane 183 20 354 26 12.29067 2 1 108 70
629 Bernardina 40 33 236 48 3.76360 91 48
631 Philippina 183 –2 5.90220 6 2 171 38
685 Hermia 197 87 29 79 50.387 93 148
695 Bella 87 –55 314 –56 14.21900 8 1 184 90 30
753 Tiflis 5 36 199 57 9.8259 129 64
800 Kressmannia 345 37 172 34 4.460963 8 2 108 51
808 Merxia 26 54 192 57 30.630 4 1 158 87 32
810 Atossa 12 67 188 69 4.38547 99 71 60
825 Tanina 46 48 231 60 6.93981 2 1 114 40
832 Karin 242 46 59 44 18.3512 13 3 84 39
847 Agnia 341 18 162 13 14.8247 3 1 136
889 Erynia 187 –60 335 –74 9.8749 94 65
925 Alphonsina 296 41 147 22 7.87754 4 1 134 48 79
934 Thuringia 120 –52 8.16534 123 59
1002 Olbersia 220 35 16 54 10.2367 87 48 54
1087 Arabis 334 –7 155 12 5.79501 3 1 156 92
1102 Pepita 25 –34 231 –30 5.10532 147 47
1140 Crimea 12 –73 175 –22 9.7869 3 1 96 116
1148 Rarahu 148 –9 322 –9 6.54449 95 64
1207 Ostenia 310 –77 124 –51 9.07129 2 2 87 71
1291 Phryne 106 35 277 59 5.58414 2 1 129 72
1301 Yvonne 39 41 7.31968 78 56 33
1333 Cevenola 38 –86 220 –44 4.87932 3 1 104 91
1382 Gerti 268 23 87 28 3.081545 2 1 60 56 52
1419 Danzig 22 76 193 62 8.11957 1 1 135 87
1482 Sebastiana 262 –68 91 –67 10.48965 2 1 131 39 30
1514 Ricouxa 251 75 68 69 10.42468 3 1 68 56
1568 Aisleen 109 –68 6.67597 82 37
1635 Bohrmann 5 –38 185 –36 5.86427 8 1 108 47
1659 Punkaharju 259 –71 75 –22 5.01327 2 1 118 66
1682 Karel 232 32 51 41 3.37485 54 84 36
1709 Ukraina 165 –61 2 –40 7.30517 2 1 46 79
1742 Schaifers 198 57 47 55 8.53270 3 1 106
1747 Wright 227 31 5.28796 70 55
1889 Pakhmutova 22 –76 167 –40 17.5157 68 46 35
1930 Lucifer 32 17 211 –19 13.0536 6 1 106 43 66
2156 Kate 49 74 5.62215 4 1 44
3678 Mongmanwai 125 –65 4.18297 2 1 103 31
4483 Petofi 107 40 4.33299 3 1 36

Notes. For each asteroid, the table gives also the number of dense lightcurves Nlc observed during Napp apparitions and the number of sparse data points for the corresponding observatory: N689, N699, N703, NE12, NG96, N950 and NHip. Pole solutions preferred by asteroid occultation measurements (Ďurech et al. 2011) are emphasized by a bold font.

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