Open Access
Table 4
Median abundance [X/Fe] difference between GALAH, APOGEE, and WG15 for the sample of stars in common.
| Element | GALAH − WG15 | APOGEE − WG15 | ||
|---|---|---|---|---|
| offset | std dev | offset | std dev | |
| C I | 0.16 | 0.35 | 0.01 | 0.31 |
| O I | −0.05 | 0.36 | −0.09 | 0.15 |
| Na I | 0.01 | 0.19 | −0.08 | 0.34 |
| Mg I | −0.01 | 0.18 | −0.01 | 0.16 |
| Al I | 0.04 | 0.22 | −0.12 | 0.17 |
| Si I | 0.04 | 0.24 | −0.02 | 0.22 |
| S I | 0.33 | 0.76 | ||
| Ca I | 0.11 | 0.23 | 0.02 | 0.19 |
| Sc I | 0.10 | 0.17 | ||
| Ti I | 0.03 | 0.23 | −0.02 | 0.22 |
| Ti II | −0.05 | 0.25 | ||
| V I | 0.13 | 0.35 | ||
| Cr I | 0.02 | 0.24 | 0.03 | 0.31 |
| Mn I | 0.00 | 0.32 | 0.04 | 0.22 |
| Co I | 0.06 | 0.42 | −0.01 | 0.29 |
| Ni I | 0.04 | 0.22 | 0.02 | 0.16 |
| Cu I | 0.09 | 0.23 | ||
| Zn I | 0.04 | 0.29 | ||
| Y II | −0.03 | 0.39 | ||
| Zr I | 0.12 | 0.52 | ||
| Mo I | 0.15 | 0.37 | ||
| Ba II | 0.10 | 0.36 | ||
| La II | 0.06 | 0.34 | ||
| Ce II | 0.07 | 0.32 | 0.03 | 0.18 |
| Nd II | 0.17 | 0.39 | ||
| Sm II | −0.05 | 0.44 | ||
| Eu II | −0.05 | 0.22 | ||
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