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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

Notes. Equivalent diameters from occultation and AO fits are also shown. The numbers in bold face indicate that the values of the beaming parameter for those fits were fixed to a default value. If several radiometric values are available, we have kept them in the same column, separated by commas.

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