Table A.4.
Physical properties of asteroids with new rotation period determinations based on the V-band ASAS-SN data.
| Asteroid | P | M | NA | D | |
|---|---|---|---|---|---|
| [hours] | [km] | ||||
| 835 | Olivia | 1104.0 | C | 145 | 30.4 |
| 991 | McDonalda | 339.5 | E | 178 | 38.6 |
| 1034 | Mozartia | 449.9 | E | 216 | 9.7 |
| 1445 | Konkolya | 59.395 | C | 96 | 20.3 |
| 1714 | Sy | 317.8 | E | 193 | 14.0 |
| 1745 | Ferguson | 1078.2 | C | 136 | 12.1 |
| 1755 | Lorbach | 7.9765 | CE | 208 | 24.9 |
| 1787 | Chiny | 13.5609 | E | 173 | 19.9 |
| 1984 | Fedynskij | 8.1405 | E | 187 | 38.4 |
| 2027 | Shen Guo | 1117.3 | E | 164 | 16.5 |
| 2051 | Chang | 12.0142 | CE | 183 | 16.4 |
| 2138 | Swissair | 369.7 | C | 244 | 12.9 |
| 2158 | Tietjen | 8.6581 | E | 137 | 22.7 |
| 2165 | Young | 6.39009 | CE | 143 | 27.1 |
| 2191 | Uppsala | 31.317 | E | 213 | 17.5 |
| 2219 | Mannucci | 27.460 | E | 172 | 39.1 |
| 2226 | Cunitza | 189.05 | E | 159 | 14.6 |
| 2248 | Kanda | 24.736 | E | 169 | 26.4 |
| 2404 | Antarctica | 2.26238 | CE | 143 | 23.2 |
| 2405 | Welch | 14.3411 | E | 123 | 26.4 |
| 2413 | van de Hulst | 211.96 | E | 190 | 20.8 |
| 2475 | Semenov | 12.2370 | E | 131 | 14.5 |
| 2502 | Nummela | 14.3151 | E | 97 | 19.0 |
| 2660 | Wasserman | 628.3 | E | 137 | 9.2 |
| 2780 | Monnig | 681.8 | E | 91 | 4.8 |
| 2795 | Lepage | 40.368 | E | 107 | 6.1 |
| 2819 | Ensor | 161.66 | E | 130 | 9.7 |
| 2837 | Griboedov | 3.94988 | C | 119 | 12.3 |
Notes. We provide the sidereal rotational period P (its uncertainty is on the order of the last digit). The method column (M) indicates whether the rotation period was derived by the convex inversion approach (C), the ellipsoid approach (E), or both (CE). The final two columns are the number of ASAS-SN measurements NA and the size D from the MP3C database. The full table is available at the CDS.
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