Table 4.
Sample of line information.
| Stellar ID | Species | λ | χ | log gf | EW | σEW | log ϵ | Ref |
|---|---|---|---|---|---|---|---|---|
| (Å) | (eV) | (mÅ) | (mÅ) | |||||
| J003859 | O I | 7771.94 | 9.15 | 0.37 | 20.48 | 2.62 | 7.65 | 1 |
| J003859 | O I | 7774.17 | 9.15 | 0.22 | 7.73 | 1.62 | 7.24 | 1 |
| J003859 | O I | 7775.39 | 9.15 | 0.00 | 7.87 | 1.53 | 7.47 | 1 |
| J003859 | Na I | 5889.95 | 0.00 | 0.11 | 170.38 | 2.93 | 4.21 | 1 |
| J003859 | Na I | 5895.92 | 0.00 | −0.19 | 158.03 | 0.78 | 4.36 | 1 |
| J003859 | Mg I | 4167.27 | 4.35 | −0.74 | 61.95 | 1.21 | 5.66 | 1 |
| J003859 | Mg I | 4702.99 | 4.33 | −0.44 | 80.18 | 0.71 | 5.54 | 1 |
| J003859 | Mg I | 5528.40 | 4.35 | −0.55 | 79.94 | 0.72 | 5.68 | 2 |
| J003859 | Mg I | 5711.09 | 4.35 | −1.84 | 14.72 | 0.80 | 5.79 | 2 |
| J003859 | Al I | 3961.52 | 0.01 | −0.33 | 121.84 | 1.40 | 3.35 | 1 |
| J003859 | Si I | 5772.15 | 5.08 | −1.75 | 5.58 | 1.21 | 5.98 | 1 |
| J003859 | K I | 7664.90 | 0.00 | 0.12 | 65.09 | 0.89 | 3.37 | 1 |
| J003859 | K I | 7698.96 | 0.00 | −0.18 | 45.82 | 0.88 | 3.33 | 1 |
References. (1) Kramida et al. (2018a), (2) Pehlivan Rhodin et al. (2017), (3) Yu & Derevianko (2018), (4) Lawler et al. (2013), (5) Wood et al. (2013), (6) Pickering et al. (2001, 2002), (7) Sobeck et al. (2007), (8) Lawler et al. (2017), (9) Den Hartog et al. (2014), (10) O’Brian et al. (1991), (11) Belmonte et al. (2017), (12) Ruffoni et al. (2014), (13) Meléndez & Barbuy (2009), (14) Den Hartog et al. (2019), (15) Wood et al. (2014), (16) Roederer & Lawler (2012), (17) Smith et al. (1998), (18) Lawler & Dakin (1989) using hfs from Kurucz & Bell (1995), (19) Lawler et al. (2014), (20) Wood et al. (2014), (21) Den Hartog et al. (2011), (22) Lawler et al. (2015), (23) Kramida et al. (2018b), (24) Biémont et al. (2011), (25) Ljung et al. (2006), (26) Kramida et al. (2018b) using HFS/IS from McWilliam (1998), (27) Lawler et al. (2001a) using HFS from Ivans et al. (2006), (28) Den Hartog et al. (2003) using HFS/IS from Roederer et al. (2008), (29) Lawler et al. (2001b) using HFS/IS from Ivans et al. (2006), (30) Wickliffe et al. (2000), (31) Lawler et al. (2008), (32) Sneden et al. (2009), (33) Kramida & Ralchenko (1999) using hfs from Kurucz & Bell (1995). The full table is available at the CDS.
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