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Table 4.
Number of confirmed isolated U and Ne lines with S/N higher than ten found in the 12 U–Ne spectra for NIR wavelengths.
| HCL HKH | UI | UII | NeI | NeII | IU |
|---|---|---|---|---|---|
| 0120 | 273 | 11 | 158 | 40 | 0.74 |
| 0121 | 377 | 12 | 151 | 39 | 1.08 |
| 0122 | 294 | 9 | 153 | 43 | 0.80 |
| 0123 | 334 | 12 | 158 | 44 | 0.95 |
| 0124 | 351 | 13 | 145 | 39 | 1.04 |
| 0125 | 307 | 9 | 162 | 40 | 0.82 |
| 0126 | 295 | 13 | 155 | 42 | 0.80 |
| 0127 | 503 | 11 | 153 | 40 | 1.39 |
| 0128 | 366 | 10 | 144 | 45 | 1.12 |
| 0129 | 398 | 12 | 154 | 39 | 1.09 |
| 0130 | 315 | 13 | 157 | 42 | 0.83 |
| 0131 | 478 | 11 | 143 | 41 | 1.35 |
The last column contains the average of the U line intensity normalized to the average of its line intensity in the 12 spectra (IU).
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