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Table 2
Sizes of several asteroids based on radiometry from this work, U11/H13, and NEOWISE (DW ; Mainzer et al. 2016), and those determined from ellipsoids fitted to stellar occultation chords (compiled by Dunham et al. 2016), and based on adaptive optics (AO; Hanuš et al. 2017a,b).
Asteroid | D(km) | DU 11 (km) | DW (km) | Occ. a × b (km) | DOcc,eq (km) | AO a × b × c (km) | DAO,eq (km) |
---|---|---|---|---|---|---|---|
(9) | 223, 160 | 166 | 183, 184 | 176 × 161 | 168 | – | 168 |
200 × 137 | 166 | ||||||
182 × 153 | 167 | ||||||
(10) | 454, 403 | 428 | 533 | 464 × 383 | 422 | – | 412 |
(16) | 200, 236 | 207 | 288 | 235 × 230 | 233 | – | 225 |
(130) | 212, 212 | 183 | 181,162, 159 | 255 × 154 | 199 | 262 × 205 × 164 | 206 |
(303) | 107, 89 | 99,105 | 104, 125 | 87 × 110 | 98 | – | – |
(1263) | 50, 44 | 51 | 40.2, 37.56 | 53.9 × 36.2 | 44 | – | – |
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