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Table 8.
Comparison of our integrated-light NLTE abundance measurements with NLTE measurements for individual stars (Kovalev et al. 2019, K2019).
| [Fe/H] | [Mg/Fe] | [Ti/Fe] | |
|---|---|---|---|
| K2019 | |||
| NGC 104 | −0.74 ± 0.03 | +0.38 ± 0.05 | +0.30 ± 0.07 |
| NGC 362 | −1.05 ± 0.04 | +0.15 ± 0.06 | +0.29 ± 0.06 |
| NGC 6752 | −1.48 ± 0.06 | +0.20 ± 0.09 | +0.17 ± 0.07 |
| NGC 7078 | −2.28 ± 0.06 | +0.22 ± 0.19 | +0.21 ± 0.05 |
| This work (from Table C.1) | |||
| NGC 104 | −0.74 ± 0.02 | +0.40 ± 0.06 | +0.41 ± 0.03 |
| NGC 362 | −1.07 ± 0.02 | +0.17 ± 0.03 | +0.42 ± 0.03 |
| NGC 6752 | −1.70 ± 0.01 | +0.31 ± 0.07 | +0.36 ± 0.03 |
| NGC 7078 | −2.29 ± 0.02 | +0.15 ± 0.04 | +0.43 ± 0.05 |
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