Table 2.
Summary of the different combinations of asteroseismic and spectroscopic constraints used in this study for the fields considered: Kepler, K2 (C01-08, C10-18), and TESS-SCVZ.
| Fields | Seismo. | Spectro. | N | ⟨Δϖ⟩ (μas) | ⟨Δϖcorr⟩ (μas) | Full range | Full range (corr.) |
|---|---|---|---|---|---|---|---|
| Kepler | MA09 | APOGEE DR17 | 4687 | −32 ± 0.4 | −12 ± 0.4 | – | – |
| E20 | – | – | −20 ± 0.3 | −0.4 ± 0.3 | – | – | |
| K2 | MA09 | APOGEE DR17 | 7024 |
 |
 |
[−43, +2] | [−6, +33] |
| E20 | – | – |
 |
 |
[−39, +1] | [−4, +32] | |
| MA09 | GALAH DR3 | 5919 |
 |
 |
[−68, +4] | [−41, +32] | |
| E20 | – | – |
 |
 |
[−70, +15] | [−45, +43] | |
| TESS-SCVZ | MA09 | APOGEE DR17 | 1253 | −23 ± 1.2 | −15 ± 1.2 | – | – |
| E20 | – | – | −41 ± 1.4 | −33 ± 1.4 | – | – | |
Notes. The median parallax offsets obtained before applying L21 corrections (Δϖ=ϖEDR3 − ϖPARAM) and after (Δϖcorr = ϖEDR3, corr − ϖPARAM) are indicated. For K2, the median offset is calculated considering the 17 campaigns together, and the uncertainty quoted corresponds to the 16th and 84th percentiles. In addition, the full range with the minimum and maximum offsets measured for K2 fields is also given.
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