Table C.1.
Spectroscopic atmospheric parameters, and abundances, for the RG in KIC 10001167, both ours (FIES) and from the APOGEE DR17 near-infrared survey.
| Quantity | APOGEE DR17a,b | FIESa, astrophysical log(gf) | FIESa, laboratory log(gf) |
|---|---|---|---|
| (Slumstrup et al. 2019) | (Stetson & Pancino 2008) | ||
| Teff(K) | 4598(8) | 4622(36) | 4698(68) |
| log g(cgs) | 2.209 | fixed 2.20 | fixed 2.20 |
| [FeI/H] (dex) | −0.677(9)c | −0.726(66) | −0.672(99) |
| [FeII/H] (dex) | −0.786(67) | −0.877(74) | |
| [α/Fe] (dex) | 0.277(8) | 0.369(69) | 0.319(100) |
| ξ(km s−1) | 1.230(60) | 1.290(70) | |
| nFeI | 73 | 68 | |
| nFeII | 12 | 12 | |
| [NaI/Fe] | 0.067(88) | 0.267(67), n = 2 | 0.230(99), n = 2 |
| [MgI/Fe] | 0.339(15) | 0.412(68), n = 3 | 0.463(99), n = 2 |
| [AlI/Fe] | 0.302(21) | 0.404(78), n = 2 | 0.419(102), n = 2 |
| [SiI/Fe] | 0.248(16) | 0.379(66), n = 5 | 0.190(103), n = 7 |
| [CaI/Fe] | 0.194(19) | 0.254(84), n = 5 | 0.249(100), n = 3 |
| [TiI/Fe] | 0.150(23) | 0.429(95), n = 11 | 0.373(108), n = 8 |
| [TiII/Fe] | 0.375(83) | 0.379(76), n = 2 | 0.305(99), n = 2 |
| [CrI/Fe] | −0.055(54) | 0.106(80), n = 5 | 0.036(117), n = 5 |
| [Mn/Fe] | −0.150(20) | ||
| [NiI/Fe] | 0.087(16) | 0.102(86), n = 8 | 0.081(121), n = 9 |
Notes. Solar reference for the FIES abundances is Asplund et al. (2009), while for APOGEE DR17 it is Grevesse et al. (2007). The number of lines used for each FIES abundance measurement is referred to as "n" (including nFeI(I)). ξ refers to the atmospheric micro-turbulent velocity. The abundance uncertainty estimates for FIES are the standard deviation of the individual lines against the mean, and not the standard errors.
For APOGEE DR17, all measurements are "overall" abundances X instead of uniquely atomic neutral XI or single-ionised XII, with the exception of [TiII/Fe] (atomic single-ionised). For the rest of the elements, whether the APOGEE abundances are marked [X/Fe] or [XI/Fe] has no bearing on the actual state.
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