Table A.1
Properties of asteroids regarded in Section 4.
| Name | Family | Barbarian | Group | Source |
|---|---|---|---|---|
| 1987 VT | Watsonia | LM | 1 | |
| 1992 OB | Tirela | LL | 1 | |
| 1997 AK17 | Brangane | LL | 1 | |
| 2001 CD42 | Tirela | LL | 1 | |
| Anastasia | Yes | LL | 2 | |
| Aquitania | Aquitania | Yes | LL | 2 |
| Barbara | Yes | LL | 2 | |
| Baucis | Yes | LL | 3 | |
| Brangane | Brangane | Yes | LM | 2 |
| Chloe | Yes | LM | 2 | |
| Crabeels | Scania | LL | 2 | |
| Haremari | Watsonia | Yes | LM | 3 |
| Henan | Scania | Yes | LL | 2 |
| Hercynia | Yes | LL | 3 | |
| Honoria | Yes | LM | 2 | |
| Kiladze | Scania | LL | 2 | |
| Lavrov | Scania | LL | 3 | |
| Luisa | Aquitania | Yes | LM | 4 |
| Lujiaxi | Scania | LL | 2 | |
| Molaro | Aquitania | LL | 1 | |
| Pax | Yes | LM | 2 | |
| Pax | Yes | LM | 5 | |
| Raybrown | Scania | LL | 2 | |
| Scania | Scania | LL | 2 | |
| Tokio | LM | 6 | ||
| Valeria | Yes | LM | 3 | |
| Waland | Scania | LL | 2 | |
| Watsonia | Watsonia | Yes | LM | 2 |
| Welther | Aquitania | LM | 1 | |
| Yurilvovia | Scania | LL | 3 |
Notes. For each asteroid, we indicate its dynamical family, whether it is a confirmed Barbarian (following Devogèle et al. (2018), blank: undetermined), its LL/LM association defined in this work, and the source publication of its spectrum. 1 – This work, 2 – DeMeo et al. (2009), 3 Devogèle et al. (2018), 4 – Sunshine et al. (2008), 5 – Binzel et al. (2019), and 6 – Fornasier et al. (2010).
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