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Table 2
Comparison of the spectroscopic parameters from VWA with photometric values from KIC and from the asteroseismic analysis of 14 Kepler giants.
| VWA | KIC | Asteroseis. | ||||||||
| KIC-ID | Teff | log g | [Fe/H] | Teff | log g | [Fe/H] | Teff | log g | ||
|
|
||||||||||
| 1726211 | 4950 ± 70 | 2.36 ± 0.26 | −0.66 ± 0.08 | 4837 ± 200 | 2.68 ± 0.50 | −0.96 ± 0.50 | 4627 ± 103 | 2.37 ± 0.04 | ||
| 2714397 | 5000 ± 70 | 2.65 ± 0.25 | −0.40 ± 0.08 | 4881 ± 200 | 2.52 ± 0.50 | −0.53 ± 0.50 | 4762 ± 99 | 2.41 ± 0.01 | ||
| 3744043 | 5020 ± 70 | 3.08 ± 0.25 | −0.25 ± 0.08 | 4994 ± 200 | 2.50 ± 0.50 | −0.09 ± 0.50 | 4769 ± 115 | 2.95 ± 0.02 | ||
| 3860139 | 4550 ± 90 | 2.23 ± 0.25 | + 0.25 ± 0.13 | 4589 ± 200 | 2.22 ± 0.50 | + 0.60 ± 0.50 | ||||
| 3936921 | 4580 ± 90 | 2.19 ± 0.27 | + 0.29 ± 0.10 | 4436 ± 200 | 2.38 ± 0.50 | −0.06 ± 0.50 | 4587 ± 54 | 2.33 ± 0.04 | ||
| 4157282 | 4450 ± 90 | 1.88 ± 0.35 | + 0.10 ± 0.13 | 4344 ± 200 | 2.13 ± 0.50 | −0.78 ± 0.50 | ||||
| 4177025 | 4390 ± 90 | 1.85 ± 0.29 | −0.25 ± 0.11 | 4346 ± 200 | 2.14 ± 0.50 | −0.49 ± 0.50 | ||||
| 5709564 | 4775 ± 70 | 2.46 ± 0.25 | −0.22 ± 0.08 | 4752 ± 200 | 2.52 ± 0.50 | −0.06 ± 0.50 | 4718 ± 118 | 2.33 ± 0.04 | ||
| 7006979 | 4770 ± 70 | 2.23 ± 0.25 | −0.36 ± 0.08 | 4891 ± 200 | 2.21 ± 0.50 | −0.01 ± 0.50 | 4645 ± 103 | 2.45 ± 0.05 | ||
| 8017159 | 4625 ± 70 | 1.19 ± 0.25 | −2.01 ± 0.08 | 4634 ± 200 | 2.45 ± 0.50 | −1.07 ± 0.50 | ||||
| 8476245 | 4865 ± 70 | 1.92 ± 0.25 | −1.33 ± 0.09 | 4817 ± 200 | 2.76 ± 0.50 | −1.20 ± 0.50 | ||||
| 10403036 | 4485 ± 70 | 2.00 ± 0.25 | −0.58 ± 0.09 | 4388 ± 200 | 2.21 ± 0.50 | −1.39 ± 0.50 | ||||
| 10426854 | 4955 ± 80 | 2.49 ± 0.27 | −0.31 ± 0.10 | 4731 ± 200 | 2.57 ± 0.50 | −1.03 ± 0.50 | ||||
| 11342694 | 4695 ± 100 | 2.75 ± 0.27 | + 0.53 ± 0.11 | 4603 ± 200 | 2.65 ± 0.50 | + 0.50 ± 0.50 | 4670 ± 90 | 2.78 ± 0.02 | ||
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