Table C.1.
Parallax zero points, measured as the difference between the Gaia EDR3 and the asteroseismic parallaxes (ϖGEDR3 − ϖPARAM) for the asteroseismic fields considered in this study.
| Field | MA09+APOGEE | E20+APOGEE * | MA09+GALAH | E20+GALAH |
|---|---|---|---|---|
| Kepler | −32.02 ± 0.36 (4687) | −20.09 ± 0.33 (4687) | - | - |
| K2 C01 | −18.32 ± 3.00 (201) | −21.45 ± 3.00 (201) | −14.2 ± 2.93 (240) | −14.84 ± 2.87 (240) |
| K2 C02 | −22.81 ± 2.11 (386) | −22.21 ± 2.28 (386) | −28.28 ± 1.81 (620) | −28.64 ± 1.89 (620) |
| K2 C03 | −8.18 ± 2.05 (543) | −6.01 ± 2.07 (543) | −3.4 ± 2.82 (262) | −5.23 ± 2.88 (262) |
| K2 C04 | −14.16 ± 1.42 (1092) | −18.30 ± 1.43 (1092) | −17.68 ± 2.48 (474) | −21.39 ± 2.55 (474) |
| K2 C05 | −15.50 ± 1.41 (865) | −13.59 ± 1.46 (865) | −12.46 ± 1.65 (757) | −12.39 ± 1.65 (757) |
| K2 C06 | −22.04 ± 1.56 (690) | −21.20 ± 1.60 (690) | −10.82 ± 2.72 (262) | −16.51 ± 2.53 (262) |
| K2 C07 | −18.29 ± 1.91 (422) | −20.03 ± 1.99 (422) | −20.67 ± 1.42 (822) | −21.41 ± 1.46 (822) |
| K2 C08 | −18.78 ± 2.24 (436) | −21.11 ± 2.35 (436) | −15.7 ± 4.0 (159) | −17.65 ± 3.89 (159) |
| K2 C10 | −2.08 ± 3.59 (199) | −5.65 ± 3.49 (199) | −12.58 ± 4.07 (117) | −11.07 ± 3.99 (117) |
| K2 C11 | −42.82 ± 3.56 (189) | −39.15 ± 3.66 (189) | −68.18 ± 4.79 (235) | −69.92 ± 4.81 (235) |
| K2 C12 | 2.49 ± 2.36 (462) | 1.39 ± 2.22 (462) | −10.77 ± 6.5 (63) | −10.43 ± 6.43 (63) |
| K2 C13 | −30.99 ± 2.03 (423) | −33.12 ± 2.06 (423) | −37.89 ± 2.03 (645) | −37.05 ± 1.99 (645) |
| K2 C14 | −28.68 ± 2.65 (354) | −26.89 ± 2.41 (354) | −23.9 ± 4.00 (123) | −16.16 ± 4.04 (125) |
| K2 C15 | −11.46 ± 13.08 (10) | −7.54 ± 11.21 (10) | −14.58 ± 1.78 (735) | −7.48 ± 1.62 (735) |
| K2 C16 | −23.36 ± 2.60 (310) | −21.32 ± 2.52 (310) | −13.83 ± 3.29 (201) | −8.53 ± 3.16 (201) |
| K2 C17 | −17.95 ± 2.32 (348) | −18.84 ± 2.42 (348) | −11.78 ± 3.81 (162) | −11.53 ± 3.66 (162) |
| K2 C18 | −10.36 ± 5.27 (94) | −2.56 ± 5.55 (94) | 4.08 ± 6.81 (78) | 15.23 ± 6.35 (78) |
| TESS | −23.23 ± 1.27 (1253) | −41.43 ± 1.43 (1253) | - | - |
Notes. Each column corresponds to a different combination of asteroseismic (MA09 or E20) and spectroscopic (APOGEE or GALAH) constraints. The offsets reported are given in μas, and the column used in Sects. 4 and 5 is followed by an asterisk. The number of stars is indicated in brackets. See Sect. 2 for more details about the samples.
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