Table A.2.
Physical properties of asteroids with new shape model determinations based on the V-band ASAS-SN data.
| Asteroid | λ1 | β1 | λ2 | β2 | P | M | NA | PLCDB | D | ||
|---|---|---|---|---|---|---|---|---|---|---|---|
| [deg] | [deg] | [deg] | [deg] | [hours] | [hours] | [km] | |||||
| 59 | Elpis | 300 | −55 | 13.6747 | CE | 289 | 13.67 | 3 | 165.1 | ||
| 70 | Panopaea | 40 | 26 | 233 | 24 | 15.8041 | C | 314 | 15.81 | 3 | 127.9 |
| 74 | Galatea | 109 | 1 | 289 | 14 | 17.2675 | C | 327 | 17.27 | 3 | 113.1 |
| 83 | Beatrix | 182 | −9 | 10.1107 | E | 351 | 10.16 | 3 | 89.6 | ||
| 105 | Artemis | 47 | 24 | 37.118 | C | 405 | 37.15 | 3 | 119.0 | ||
| 106 | Dione | 57 | 12 | 237 | 1 | 16.2126 | C | 379 | 16.21 | 3 | 153.4 |
| 126 | Velleda | 120 | 46 | 300 | 32 | 5.36708 | C | 249 | 5.37 | 3 | 43.9 |
| 131 | Vala | 58 | 34 | 244 | 17 | 5.18072 | C | 368 | 5.18 | 3 | 31.3 |
| 133 | Cyrene | 155 | −59 | 348 | −52 | 12.7086 | CE | 303 | 12.71 | 3 | 72.2 |
| 134 | Sophrosyne | 100 | 35 | 276 | 7 | 17.1893 | CE | 293 | 17.20 | 3 | 112.2 |
| 137 | Meliboea | 173 | −7 | 355 | 13 | 25.673 | C | 316 | 25.68 | 3 | 128.7 |
| 139 | Juewa | 96 | −1 | 271 | −25 | 20.9846 | C | 279 | 20.99 | 3 | 151.1 |
| 140 | Siwa | 88 | −27 | 265 | −27 | 34.398 | CE | 320 | 34.45 | 3 | 110.6 |
| 168 | Sibylla | 108 | −62 | 47.015 | CE | 348 | 47.01 | 3 | 145.4 | ||
| 240 | Vanadis | 64 | 12 | 247 | 16 | 10.5606 | C | 349 | 10.64 | 3 | 87.9 |
| 248 | Lameia | 116 | 18 | 292 | 27 | 11.9120 | C | 332 | 11.91 | 3 | 50.1 |
| 261 | Prymno | 150 | 46 | 334 | 34 | 7.9998 | C | 327 | 8.00 | 3 | 50.0 |
| 326 | Tamara | 76 | 7 | 14.4613 | CE | 306 | 14.45 | 3 | 89.4 | ||
Notes. We provide ecliptic coordinates λ and β of up to two pole solutions, 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 columns are the number of ASAS-SN measurements NA, the LCDB period with its reliability flag (Warner et al. 2009), the size D from the MP3C database (https://mp3c.oca.eu/catalogue/index.htm), and the DAMIT rotation state solution. The full table is available at the CDS.
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