Table A.3
CN lines responsible for and used to constrain contamination of Th and Eu features
| Wavelength (Å) | χ (eV) | log g f (dex) | Jlow | Jup | CN isotopes |
|---|---|---|---|---|---|
| 5972.985 | 0.760 | −2.05 | 32.5 | 32.5 | 12C14N a |
| 5989.054 | 0.897 | −2.23 | 41.5 | 42.5 | 12C14N b |
| 6644.304 | 0.805 | −2.25 | 14.5 | 15.5 | 12C14N a |
| 6644.352 | 0.805 | −2.66 | 15.5 | 15.5 | 12C14N a |
| 6644.922 | 1.066 | −1.97 | 59.5 | 60.5 | 12C14N a |
| 6644.965 | 1.664 | −1.95 | 31.5 | 30.5 | 13C14N a |
Notes. (a)From the line list compiled by Sneden et al. (2014) based on the measurement by Brooke et al. (2014). (b)From the online line list of Kurucz.
(a)Seismic ages for the main sample from Takeda et al. (2016). (b)Stellar parameters and seismic masses for the main sample from Takeda & Tajitsu (2015) and Takeda et al. (2016). Stellar parameters for Arcturus from Ramírez & Allende Prieto (2011).
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