Table D.1
Asteroid information used in Fig. 8b.
| Number* | Name | Bus-DeMeo type | PC4’ | Slope0.85−1.8 | Spectral file |
|---|---|---|---|---|---|
| 13 | Egeria | Ch | 0.0823 | 0.12187 | a000013.sp41aa |
| 34 | Circe | Ch | 0.0936 | 0.0999 | a000034.sp28aa |
| 41 | Daphne | Ch | 0.0606 | 0.14818 | a000041.sp70aa |
| 48 | Doris | Ch | 0.0516 | 0.04665 | a000048.sp45aa |
| 50 | Virginia | Ch | 0.0784 | 0.04637 | a000050.sp265aa |
| 78 | Diana | Ch | 0.0361 | 0.13407 | a000078.sp46aa |
| 105 | Artemis | Ch | 0.0562 | 0.12282 | a000105.sp25aa |
| 266 | Aline | Ch | 0.0612 | 0.14994 | a000266.sp44aa |
| 345 | Tercidina | Ch | 0.0522 | 0.16678 | a000345.sp45aa |
| 2099 | Opik | Ch | 0.0136 | 0.13789 | a002099.visniraa |
| 285263 | 1998 QE2 | Ch | 0.0536 | 0.0971 | a285263.visnir_xthbb |
| 452561 | 2005 AB | Ch | 0.1271 | 0.17372 | a452561.visnir_xthbb |
| 455322 | 2002 NX18 | Ch | 0.136 | 0.0647 | a455322.visnir_xthbb |
| 38 | Leda | Cgh | 0.0669 | 0.19096 | a000038.sp100aa |
| 51 | Nemausa | Cgh | 0.1138 | 0.2647 | a000051.sp29aa |
| 54 | Alexandra | Cgh | 0.058 | 0.15696 | a000054.sp259n2aa |
| 706 | Hirundo | Cgh | 0.2081 | 0.31196 | a000706.sp49aa |
| 776 | Berbericia | Cgh | 0.0204 | 0.10629 | a000776.sp38aa |
| 1300 | Marcelle | Cgh | 0.0392 | 0.15705 | a000776.sp38aa |
| 2 | Pallas | B | −0.066 | −0.07751 | a000002.sp89aa |
| 1508 | Kemi | B | −0.0687 | −0.02618 | a001508.visnirbb |
| 1580 | Betulia | B | −0.1496 | −0.06476 | a001580.visnir_xthbb |
| 2100 | Ra-Shalom | B | −0.0961 | −0.08103 | a002100.visnirbb |
| 3200 | Phaethon | B | −0.1171 | −0.14387 | a003200.visnirbb |
| 6411 | Tamaga | B | −0.0271 | −0.13471 | a006411.visnirbb |
| 17511 | 1992 QN | B | 0.0318 | − 0.11045 | a017511.visnirbb |
| 25330 | 1999 KV4 | B | 0.0836 | − 0.03163 | a025330.visnirbb |
| 101955 | Bennu | B | 0.0255 | − 0.04721 | a101955.visnirbb |
| 191 | A878 SB | Cb | −0.0065 | 0.17703 | a000191.sp38aa |
| 210 | Isabella | Cb | −0.0225 | 0.11923 | a000210.sp47aa |
| 7753 | 1988 XB | Cb | 0.0122 | 0.01477 | a007753.visnir_xthbb |
| 162173 | Ryugu | Cb | −0.1944 | 0.03318 | a162173.sp272aa |
| 1 | Ceres | C | −0.0892 | −5.3373 × 10−4 | a000001.sp41aa |
| 10 | Hygiea | C | −0.0329 | 0.16009 | a000010.sp28aa |
| 24 | Themis | C | −0.0983 | 0.02729 | a000024.sp45aa |
| 52 | Europa | C | −0.1164 | 0.15425 | a000052.sp52aa |
| 76 | Freia | C | −0.0382 | 0.24768 | a000076.sp44aa |
| 90 | Antiope | C | −0.058 | 0.19493 | a000090.sp44aa |
| 128 | Nemesis | C | −0.0326 | 0.18363 | a000128.sp263n1aa |
| 3833 | Calingasta | C | −0.0155 | 0.09164 | a003833.visnirbb |
| 65679 | 1989 UQ | C | −0.0574 | 0.04867 | a065679.visnirbb |
| 108519 | 2001 LF | C | −0.0911 | 0.0242 | a108519.visnirbb |
| 175706 | 1996 FG3 | C | −0.0789 | 0.02191 | a175706.visnirbb |
| 308635 | 2005 YU55 | C | −0.0477 | 0.12834 | a308635.visnir_xthbb |
Notes. *Asteroid samples are collected from DeMeo et al. (2009). PC4’ is calculated fourth principal component defined in DeMeo et al. (2009). Slope0.85−1.8 is slope calculated within 0.85 to 1.8 μm wavelength. Spectral files are collected from aaMIT web http://smass.mit.edu/catalog.php and bbPublished MITHNEOS Data Sets (in http://smass.mit.edu/minuspubs.html Benzel et al. (2019)).
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