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Table B.4
Differences between standard analysis and abundances based on stars in slit scan areas.
| NGC 104 | NGC 362 | NGC 6254 | NGC 6388 | NGC 6752 | NGC 7078 | NGC 7099 | |
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| Δscn−std[Fe/H] | 0.010 | −0.212 | −0.095 | −0.064 | 0.157 | −0.009 | −0.001 |
| Δscn−std[Na/Fe] | −0.001 | 0.043 | 0.044 | 0.020 | −0.043 | 0.009 | −0.005 |
| Δscn−std[Mg/Fe] | 0.017 | 0.061 | 0.034 | 0.035 | −0.044 | 0.004 | −0.003 |
| Δscn−std[Ca/Fe] | 0.003 | 0.003 | 0.015 | −0.018 | −0.011 | 0.006 | −0.006 |
| Δscn−std[Sc/Fe] | −0.010 | −0.039 | −0.045 | −0.050 | 0.029 | −0.027 | 0.001 |
| Δscn−std[Ti/Fe] | −0.001 | −0.025 | −0.038 | −0.031 | 0.052 | −0.017 | −0.007 |
| Δscn−std[Cr/Fe] | −0.008 | −0.026 | −0.007 | 0.027 | 0.031 | 0.004 | 0.003 |
| Δscn−std[Mn/Fe] | −0.012 | −0.045 | −0.006 | 0.022 | 0.006 | 0.007 | −0.007 |
| Δscn−std[Ba/Fe] | −0.002 | −0.101 | −0.079 | −0.006 | 0.132 | −0.034 | −0.008 |
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