Table A.3
List of observed spectral lines in our spectra.
| Ion | λ (Å) | log gf | Ei (eV) | Ji | Ef(eV) | Jf | log(γr) | log(γS) | log(γW) | Note |
|---|---|---|---|---|---|---|---|---|---|---|
| ... | ... | ... | ... | ... | ... | ... | ... | ... | ... | |
| Dy II | 5090.386 | −2.332 | 0.10 | 7.5 | 2.54 | 7.5 | 0.00 | 0.00 | 0.00 | New, Blend |
| Er II | 5028.905 | −2.067 | 0.05 | 5.5 | 2.52 | 6.5 | 0.00 | 0.00 | 0.00 | New |
| Lu II | 6221.891 | −1.110 | 1.54 | 2.0 | 3.53 | 1.0 | 0.00 | 0.00 | 0.00 | New |
| Th II | 5989.045 | −2.641 | 0.19 | 2.5 | 2.26 | 1.5 | 0.00 | 0.00 | 0.00 | New, Blend |
Notes. Meaning of the columns: Ion = chemical element, λ = central wavelength of the spectral line in angstrom units, Note = brief comment on the line: "New" = line not listed in previous C-MetaLL works; "N,B" = line not previously detected but typically found partially blended; "B" = line already presented in previous C-MetaLL works and typically found partially blended. A portion is shown here for guidance regarding its form and content. The machine-readable version of the full table will be published at the Centre de Données astronomiques de Strasbourg (CDS).
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