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Table 2.
Updated spin states of incorrect DAMIT models.
| Asteroid | λ1 | β1 | λ2 | β2 | P | Light curves | |
|---|---|---|---|---|---|---|---|
| Number | Name | [deg] | [deg] | [deg] | [deg] | [h] | |
| 208 | Lacrimosa | 16 | 60 | 202 | 61 | 14.08574 | Binzel (1987), Slivan & Binzel (1996), |
| Stephens (2014), USNO, Gaia DR2 | |||||||
| 526 | Jena | 16 | 50 | 194 | 54 | 11.87655 | Barucci et al. (1994), USNO, Gaia DR2 |
| 1332 | Marconia | 59 | 26 | 240 | 26 | 32.11995 | Stephens (2013), Devogèle et al. (2017), |
| USNO, Gaia DR2 | |||||||
| 4800 | Veveri | 94 | −9 | 274 | 16 | 6.214858 | Hanuš et al. (2018), Lowell, Gaia DR2 |
Notes. For each asteroid, two possible pole directions in the ecliptic coordinates (λ, β) and the sidereal rotation period P are given. Sources of light curves and sparse photometry used for model reconstruction are listed in the last column.
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