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Home All issues Volume 607 (November 2017) A&A, 607 (2017) A117 Full HTML
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Table A.1

Models diameters and uncertainty estimates.

Asteroid D rw ΔDrw D dc ΔDdc
7 Iris 8.3 220 220 217–223 213 212 209–217
12 Victoria 6.9 116 117 115–118 113 115 113–116
14 Irene 11.9 158 159 151–161 151 154 148–158
15 Eunomia 10.7 276 278 274–279 271 275 270–275
23 Thalia 15.6 114 115 113–118 126 124 120–130
24 Themis 16.2 215 225 200–243 207 211 199–229
28 Bellona 11.7 129 133 – 134 143 –
40 Harmonia 10 113 112 105–120 113 115 114–116
42 Isis 6.6 102 106 – 98 100 –
48 Doris 18.7 210 214 196–234 238 229 218–241
56 Melete 10 114 116 – 122 124 –
65 Cybele (7 im.) 21.3 297 314 288–323 285 288 281–303
65 Cybele (6 im.) 21.5 278 305 265–314 276 278 268–294
72 Feronia 8 85 86 81–94 83 83 80–95
121 Hermione (13 im.) 17.8 199 200 197–204 193 192 190–223
121 Hermione (9 im.) 18.3 193 193 189–200 193 193 188–196
146 Lucina 13.1 133 133 128–159 129 129 127–144
250 Bettina 15.8 109 111 – 116 118 –
283 Emma 12.3 148 147 142–156 136 138 134–148
354 Eleonora 16.1 162 164 151–203 172 177 165–214
511 Davida 14.9 312 313 309–315 308 309 306–315
1036 Ganymed 3.3 39 39 38–41 37 37 36–37

Notes. The mean pixel size in the AO images is (in km), Drw and Ddc are the model diameters based respectively on raw and deconvolved images with two different parametrizations. Columns ΔDrw, dc show the diameter variability estimated with the jackknife method.

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