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Table F.3.
Estimated error parameters for [Fe/H].
| Star type | epipe | σstar | σspec |
|---|---|---|---|
| The Sun | 0.008 ± 0.003 | ... | 0.008 |
| Solar-type | 0.003 ± 0.004 | 0.020 ± 0.002 | 0.016 ± 0.002 |
| F dwarfs | 0.019 ± 0.008 | 0.080 ± 0.008 | 0.034 ± 0.008 |
| FGK subg. | −0.03 ± 0.02 | 0.05 ± 0.02 | 0.06 ± 0.02 |
| Red giants | −0.07 ± 0.05 | 0.05 ± 0.05 | 0.06 ± 0.05 |
Notes. We show the best estimates of the three parameters we used in modelling the behaviour of the pipeline. We also show the offset and spectrum-to-spectrum scatter specific to the Sun.
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