Table 1.
Summary of the [Fe/H] differences between the surveys and PASTEL.
Survey | Constraint | N | MED | MAD | σSurvey | σPASTEL | Slope |
---|---|---|---|---|---|---|---|
APOGEE | 2155 | −0.01 | 0.05 | 0.01 | 0.05 | ||
APOGEE | [Fe/H] < −0.5 | 308 | 0.06 | 0.07 | 0.01 | 0.07 | |
APOGEE | [Fe/H] ≥ −0.5 | 1847 | −0.02 | 0.05 | 0.01 | 0.05 | −0.18 |
GALAH | 232 | 0.00 | 0.07 | 0.055 | 0.05 | ||
GALAH | [Fe/H] < −0.5 | 48 | 0.14 | 0.12 | 0.07 | 0.085 | |
GALAH | [Fe/H] ≥ −0.5 | 184 | −0.02 | 0.06 | 0.05 | 0.05 | |
GALAH | log g < 3.8 | 91 | 0.00 | 0.125 | 0.06 | 0.07 | |
GALAH | log g ≥ 3.8 | 141 | 0.00 | 0.05 | 0.05 | 0.05 | |
GES | 162 | 0.02 | 0.05 | 0.10 | 0.05 | ||
GES | [Fe/H] < −0.5 | 44 | 0.09 | 0.04 | 0.10 | 0.10 | |
GES | [Fe/H] ≥ −0.5 | 118 | 0.00 | 0.04 | 0.10 | 0.05 | |
RAVE | 427 | 0.01 | 0.10 | 0.135 | 0.05 | ||
RAVE | Teff < 5000 K | 177 | 0.09 | 0.13 | 0.14 | 0.07 | |
RAVE-CNN | 666 | 0.08 | 0.11 | 0.055 | 0.05 | ||
RAVE-CNN | Gmag > 9 | 150 | 0.13 | 0.19 | 0.07 | 0.06 | |
RAVE-CNN | [Fe/H] < −0.5 | 336 | 0.18 | 0.14 | 0.07 | 0.07 | |
RAVE-CNN | [Fe/H] ≥ −0.5 | 330 | 0.01 | 0.07 | 0.04 | 0.05 | −0.32 |
LAMOST | 1767 | 0.00 | 0.055 | 0.03 | 0.05 | ||
LAMOST | [Fe/H] < −0.5 | 136 | 0.08 | 0.095 | 0.025 | 0.07 | |
LAMOST-Payne | 2243 | −0.07 | 0.07 | 0.03 | 0.05 | −0.17 | |
LAMOST-Payne | [Fe/H] < −0.5 | 246 | 0.15 | 0.16 | 0.05 | 0.08 | |
SEGUE | 181 | 0.07 | 0.16 | 0.04 | 0.10 | ||
SEGUE | [Fe/H] < −2 | 111 | 0.17 | 0.16 | 0.05 | 0.10 | |
SEGUE | [Fe/H] ≥ −2 | 70 | −0.045 | 0.085 | 0.03 | 0.07 |
Notes. Differences are measured with the median value, MED, and the dispersion, MAD, for the N common stars with various constraints. The typical (median) [Fe/H] uncertainty listed in each catalogue for the corresponding selected stars is also given. When relevant, the slope of the linear fit on the distribution of the residuals versus [Fe/H] is provided.
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