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Table 4.
Comparison between the method used in Mombarg et al. (2019) and in this work.
| Asteroseismic | Spectroscopic | Z | GaiaL | |
|---|---|---|---|---|
| input | Teff and log g | |||
| This work | Pn | A posteriori | Fixed to value | A posteriori |
| cutoff | from spectroscopy | cutoff | ||
| Mombarg et al. (2019) | Π0 | Fitted | Fixed to 0.014 | Not included |
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