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This article has an erratum: [https://doi.org/10.1051/0004-6361/202453645e]


Table 1

Lines studied in the H-band.

Species λ (Å) χex (eV) log gf Smith13 log gf (VALD3) log gf (NIST)
Mg I 15 740.716 5.931 −0.262 −0.323 −0.212
15 748.988 5.932 0.276 0.049 −0.338
15 765.842 5.933 0.504 0.320 −0.337
15 879.521 5.946 −1.248 −2.102 −1.998
15 886.261 5.946 −1.555 −1.742 −1.521
Al I 16718.957 4.085 0.290 0.152 0.220
16750.539 4.088 0.408
16763.359 4.087 −0.524 −0.550 −0.480
Si I 15 376.831 6.222 −0.649 −0.701
15 960.063 5.984 0.107 0.130 0.197
16060.009 5.954 −0.566 −0.452 −0.429
16094.787 5.964 −0.168 −0.088 −0.078
16215.670 5.964 −0.665 −0.565 −0.575
16680.770 5.984 −0.140 −0.138 −0.090
16828.159 5.984 −1.102 −1.058 −1.012
Ca I 16150.763 4.532 −0.229 0.362
16155.236 4.532 −0.619 −0.758
16157.365 4.554 −0.208 −0.219
16197.075 4.535 0.089
16204.087 4.535 −0.627

Notes. Oscillator strengths, log gf, reported in Smith et al. (2013), Smith et al. (2021), or given in VALD3 or Kurucz (1993), (1995 Atomic Line Data (R. L. Kurucz and B. Bell) Kurucz CD-ROM No. 23. Cambridge, Mass.: Smithsonian Astrophysical Observatory) and NIST are reported.

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