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Table A.3.

Physical properties of asteroids with revised shape model determinations based on the V-band ASAS-SN data and comparison with the DAMIT database.

Asteroid λ1 β1 λ2 β2 P M NA PLCDB D λD1 βD1 λD2 βD2 PD
[deg] [deg] [deg] [deg] [hours] [hours] [km] [deg] [deg] [deg] [deg] [hours]
5 Astraea 84 52 270 44 16.8006 CE 312 16.81 3 108.3 124 39 16.8006
12 Victoria 170 37 8.6604 C 347 8.66 3 115.1 178 −28 8.6603
13 Egeria 34 46 7.04664 C 262 7.04 3 227.0 54 34 233 6 7.04667
16 Psyche 35 −11 215 16 4.19597 C 377 4.20 3 207.2 36 −10 4.19595
17 Thetis 55 12 237 21 12.2660 CE 290 12.27 3 84.9 236 19 12.2660
19 Fortuna 102 51 283 59 7.4432 CE 252 7.44 3 196.4 97 69 7.4432
20 Massalia 122 46 302 47 8.0976 CE 312 8.10 3 131.6 179 39 360 40 8.0990
21 Lutetia 52 −3 232 −0 8.1683 CE 300 8.17 3 108.4 52 −6 8.1683
23 Thalia 340 −70 12.3122 CE 304 12.31 3 106.2 158 −46 343 −74 12.3124
25 Phocaea 342 9 9.9353 CE 334 9.93 3 83.2 347 10 9.9354
28 Bellona 103 −10 282 4 15.7078 CE 362 15.71 3 97.4 98 −10 15.7079

Notes. We provide ecliptic coordinates λ and β of up to two pole solutions, sidereal rotational period P (its uncertainty is of the order of the last digit). The method (M) column indicates whether the rotation period was derived by the convex inversion (C), ellipsoid (E) approach, or both (CE) approaches. The final columns are the number of ASAS-SN measurements NA, the LCDB period with its reliability flag (Warner et al. 2009) and the size D from the MP3C database3. The full table is available at the CDS.

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