Table 3
Visible spectra parameters of the analysed asteroids.
| Asteroid | Slope A | Slope A corr | Slope B | App. depth | Tax. | M4AST | SMASS |
|---|---|---|---|---|---|---|---|
| (%/0.1 μm) | (%/0.1 μm) | (%/0.1 μm) | |||||
| 2275 | 15.28 ± 0.70 | 13.99 ± 0.70 | −29.59 ± 1.57 | 1.468 ± 0.026 | V | R or Sa | |
| 2452 | 14.66 ± 0.46 | 13.71 ± 0.46 | −26.50 ± 3.64 | 1.532 ± 0.047 | V | V | V |
| 3188 | 13.40 ± 1.21 | 12.41 ± 1.21 | −25.02 ± 9.44 | 1.743 ± 0.123 | V | V | |
| 3331 | 15.36 ± 0.67 | 10.17 ± 0.67 | −35.19 ± 4.57 | 1.841 ± 0.122 | V | V | |
| 4693 | 14.84 ± 0.37 | 10.84 ± 0.37 | −31.21 ± 6.45 | 1.597 ± 0.160 | V | V | |
| 5524 | 17.73 ± 0.86 | 12.84 ± 0.86 | −33.24 ± 5.07 | 1.609 ± 0.036 | V | R or Sa | |
| 7223 | 20.69 ± 0.43 | 15.17 ± 0.43 | −34.65 ± 5.57 | 1.664 ± 0.128 | V | R or V | |
| 7302 | 11.37 ± 0.24 | 10.70 ± 0.24 | −12.78 ± 1.78 | 1.157 ± 0.030 | S | S | S |
| 9007 | 12.88 ± 1.15 | 8.56 ± 1.15 | −33.64 ± 4.75 | 1.558 ± 0.155 | V | V | |
| 14390 | 6.31 ± 1.40 | 5.44 ± 1.40 | −24.78 ± 1.97 | 1.685 ± 0.043 | ? | V or O | V |
| 19983 | 19.21 ± 2.87 | 16.54 ± 2.87 | −27.20 ± 1.39 | 1.426 ± 0.105 | V | R or Sa | |
| 29733 | 10.24 ± 1.07 | 9.76 ± 1.07 | −24.80 ± 3.27 | 1.761 ± 0.093 | V | V | |
| 51742 | 10.34 ± 0.52 | 9.37 ± 0.52 | −24.01 ± 6.07 | 1.710 ± 0.066 | V | V | |
| 90223 | 7.94 ± 0.72 | 6.73 ± 0.72 | −25.73 ± 4.89 | 1.985 ± 0.101 | V | V |
Notes. Columns are: Slope A, Slope B, Slope A corr – which is Slope A corrected for the phase angle effect, and the apparent depth. The closest taxonomic type is given based on the measured parameters (Tax.), using the M4AST tool (Popescu et al. 2012) and for asteroids with NIR spectra also using the SMASS tool.
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