Table A.1
References of the asteroid spectra used in this study.
| Number | Name | M22 | DM09 | Bar. | Reference |
|---|---|---|---|---|---|
| 15 | Eunomia | K (80%), S (20%) | K | No | DeMeo et al. (2009) |
| 172 | Baucis | L (95%) | L | Yes | Devogèle et al. (2018) |
| 221 | Eos | K (71%), M (21%), S (8%) | Cb | No | (a) Xu et al. (1995), Clark et al. (2009) |
| K | K | (b) DeMeo et al. (2009) | |||
| 234 | Barbara | L (90%), M (10%) | L | Yes | (a) Xu et al. (1995), Gietzen et al. (2012) |
| L (71%), S (29%) | L | (b) DeMeo et al. (2009) | |||
| 236 | Honoria | M (87%), P (6%), K (4%) | L | Yes | DeMeo et al. (2009) |
| 387 | Aquitania | M (85%), L (15%) | L | Yes | DeMeo et al. (2009) |
| 397 | Vienna | L (91%),M(4%) | L | - | (a) Bus & Binzel (2002b), Clark et al. (2009) |
| L | L | (b) Lazzaro et al. (2007); Clark et al. (2009) | |||
| 402 | Chloe | L (88%), M (9%) | L | Yes | DeMeo et al. (2009) |
| 458 | Hercynia | M (75%), L (13%), S (13%) | L | Yes | Devogèle et al. (2018) |
| 460 | Scania | L | L | - | DeMeo et al. (2009) |
| 579 | Sidonia | K (52%), S (47%) | K | - | DeMeo et al. (2009) |
| 599 | Luisa | L | L | Yes | (a) Binzel (2001), Clark et al. (2009) |
| L | L | (b) Xu et al. (1995), Sunshine et al. (2008) | |||
| M (82%), P (9%), S (7%) | L | (c) Bus & Binzel (2002b), Sunshine et al. (2008) | |||
| 606 | Brangane | M (77%), P (21%) | L | Yes | DeMeo et al. (2009) |
| 611 | Valeria | M (86%), P (14%) | X | Yes | Devogèle et al. (2018) |
| 653 | Berenike | K | K | - | DeMeo et al. (2009) |
| 661 | Cloelia | K (88%), M (11%) | K | - | DeMeo et al. (2009) |
| 679 | Pax | M (83%), P (6%), S (6%) | L | Yes | (a) DeMeo et al. (2009) |
| M (87%), K (8%) | L | (b) MITHNEOS (Unpublished) | |||
| 729 | Watsonia | M (87%), K (8%), P (5%) | L | Yes | DeMeo et al. (2009) |
| 742 | Edisona | K (88%), M (11%) | K | - | DeMeo et al. (2009) |
| 824 | Anastasia | L | L | Yes | DeMeo et al. (2009) |
| 980 | Anacostia | S (62%), L (20%), M (19%) | S | Yes | Bus & Binzel (2002b), Sunshine et al. (2008) |
| 1148 | Rarahu | K (86%), S (13%) | K | - | DeMeo et al. (2009) |
| 1284 | Latvia | P (59%), M (33%), S (7%) | L | Yes | Bus & Binzel (2002b), Reddy & Sanchez (2016) |
| 1372 | Haremari | P (72%), M (27%) | L | Yes | Devogèle et al. (2018) |
| 1545 | Thernoe | L | L | - | Bus & Binzel (2002b), Clark et al. (2009) |
| 1658 | Innes | L (60%), S (40%) | Sw | - | DeMeo et al. (2009) |
| 1903 | Adzhimush. | K (76%), M (20%) | K | - | DeMeo et al. (2009) |
| 2085 | Henan | L (91%),M(6%) | L | Yes | DeMeo et al. (2009) |
| 2354 | Lavrov | L | L | - | (a) Devogèle et al. (2018) |
| L (86%), S (13%) | L | (b) DeMeo et al. (2009) | |||
| 2428 | Kamenyar | K (83%), C (17%) | X | - | Vernazza et al. (2016) |
| 2957 | Tatsuo | K (51%), M (34%), S (15%) | K | - | DeMeo et al. (2009) |
| 3028 | Zhangguoxi | K | Sw | - | DeMeo et al. (2009) |
| 3043 | San Diego | L (85%), S (15%) | Sw | - | Lucas et al. (2019) |
| 3066 | McFadden | L (92%), S (8%) | Sw | - | Lazzaro et al. (2007); Fieber-Beyer et al. (2011) |
| 3734 | Waland | L (80%), M (19%) | L | - | DeMeo et al. (2009) |
| 3844 | Lujiaxi | L (90%), S (6%) | L | - | DeMeo et al. (2009) |
| 4737 | Kiladze | L | L | - | DeMeo et al. (2009) |
| 4917 | Yurilvovia | L (77%), S (12%), M (11%) | L | - | Devogèle et al. (2018) |
| 5840 | Raybrown | L (67%), M (27%), S (5%) | L | - | DeMeo et al. (2009) |
| 22771 | 1999 CU3 | L | S | - | DeMeo et al. (2009) |
| 385186 | 1994 AW1 | L | S | - | Binzel et al. (2019) |
Notes. Each line refers to one spectrum. If there are several spectra of an individual asteroid, they are denoted using (a), (b), or (c). Two references are given for a single spectrum, they refer to the visible and NIR parts respectively. Columns M22 and DM09 give the taxonomic classifications from Mahlke et al. (2022) and DeMeo et al. (2009) respectively. Barbarian (Bar.) asteroids are indicated following Devogèle et al. (2018). If the asteroid does not appear in the polarimetric database of Bendjoya et al. (2022), it is marked with a dash to indicate that the Barbarian nature is unclear.
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