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Table 1
Summary of the results obtained by matching the asteroids spectra with spectra from the Relab database.
| Spectrum | Std. dev. | Corr. coef. | Meteorite/Sample | Sample ID | Type | Texture |
|
|
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| (9147) | 0.01884 | 0.99477 | Pavlovka | MR-MJG-094 | Achondrite(AHOW) | – |
| 0.02244 | 0.99207 | Mixture | SC-EAC-039 | Pyrox Hyper Plagi Bytow Ilmen | Particulate | |
|
|
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| (99 942) | 0.01756 | 0.98013 | Simulant | CM-CMP-001-B | Soil/Lunar | Particulate |
| 0.01970 | 0.98224 | Hamlet | OC-TXH-002-C | OC-LL4 | Particulate | |
|
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| (99 942) | 0.01539 | 0.96245 | Cherokee Springs | TB-TJM-090 | OC-LL6 | Particulate |
| de-reddened | 0.01609 | 0.97272 | Cat Mountain | MB-DTB-035-A | OC-L5 | Particulate |
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| (175 706) | 0.01219 | 0.90546 | Sete Lagoas | MH-JFB-021 | OC-H4 | Slab |
| 0.01504 | 0.85366 | Murchison heated 1000 °C | MB-TXH-064-G | CC-CM2 | Particulate | |
Notes. For each asteroid, we show the best two matches, obtained by measuring the standard deviation (std. dev.) and the correlation coefficient (corr. coef.).
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