Open Access
Table 1
Stellar lines used in our analysis.
| Wavelength (Å) | log Tmax (K) | |
|---|---|---|
| C III | 1174.93 | 4.8 |
| 1175.26 | ||
| 1175.59 | ||
| 1175.71 | ||
| 1175.99 | ||
| 1176.37 | ||
| Si III | 1206.50 | 4.7 |
| O V | 1218.344 | 5.3 |
| N V | 1238.821 | 5.2 |
| 1242.804 | ||
| Si II | 1264.738 | 4.2 |
| 1265.002 | ||
| O I | 1302.168 | 3.9 |
| 1304.858 | ||
| 1306.029 | ||
| C II | 1334.532 | 4.5 |
| 1335.708 | ||
| Si IV | 1393.755 | 4.9 |
| 1402.770 |
Notes. Second column indicates rest wavelengths from the NIST Atomic Spectra Database (Kramida et al. 2016). Formation temperatures are from the Chianti v.7.0 database (Dere et al. 1997; Landi et al. 2012).
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