Table C.1
All unique identified spectral lines tracing upper atmospheres of Figs. 3, 4, 5, and 6 (thus excluding the additional lines found in Fig. 7 when using an ATES model). We give only one example reference for lines that have been previously detected.
| Wavelength (vac) (Å) | Species | Previously detected |
|---|---|---|
| 912.7 | S II | No |
| 916.7 | N II | No |
| 933.4 | S VI | No |
| 977.0 | C III | No |
| 991.6 | N III | No |
| 1021.3 | S III | No |
| 1031.9 | O VI | No |
| 1048.2 | Ar I | No |
| 1073.0 | S IV | No |
| 1122.5 | Fe III | No |
| 1199.5 | N I | No |
| 1206.5 | Si III | e.g., Linsky et al. (2010)(1) |
| 1215.7 | H I | e.g., Vidal-Madjar et al. (2003) |
| 1238.8 | N V | No |
| 1264.7 | Si II | No |
| 1302.2 | O I | e.g., Vidal-Madjar et al. (2004) |
| 1310.7 | P II | No |
| 1335.7 | C II | e.g., Vidal-Madjar et al. (2004) |
| 1358.8 | Cu II | No |
| 1393.8 | Si IV | e.g., Schlawin et al. (2010)(2) |
| 1425.0 | S I | No |
| 1548.2 | C IV | No |
| 1657.0 | C I | No |
| 1670.8 | Al II | No |
| 1850.7 | Si I | No |
| 1854.7 | Al III | No |
| 2056.3 | Cr II | No |
| 2139.2 | Zn I | No |
| 2217.2 | Ni II | No |
| 2276.2 | Ca I | No |
| 2286.9 | Co II | No |
| 2382.8 | Fe II | e.g., Sing et al. (2019) |
| 2408.0 | Co I | No |
| 2576.9 | Mn II | No |
| 2796.4 | Mg II | e.g., Fossati et al. (2010) |
| 2853.0 | Mg I | e.g., Vidal-Madjar et al. (2013)(3) |
| 3248.5 | Cu I | No |
| 3384.7 | Ti II | No |
| 3579.7 | Cr I | No |
| 3889.7 | He I | No |
| 3934.8 | Ca II | e.g., Yan et al. (2019) |
| 4227.9 | Ca I | No |
| 4255.5 | Cr I | No |
| 5170.5 | Fe II | e.g., Casasayas-Barris et al. (2019) |
| 5185.0 | Mg I | e.g., Zhang et al. (2022) |
| 5891.6 | Na I | e.g., Charbonneau et al. (2002) |
| 6564.5 | H I | e.g., Jensen et al. (2012) |
| 7667.0 | K I | e.g., Sing et al. (2011) |
| 8544.4 | Ca II | e.g., Casasayas-Barris et al. (2019) |
| 10833.3 | He I | e.g., Spake et al. (2018) |
Notes. (1)Contested by Ballester & Ben-Jaffel (2015) (2)Tentative detection (3)Contested by Cubillos et al. (2020)
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