Table 3
Identifiers and astrometric parameters for the KEYSTONE sample.
| K2 | Gaia | ||||||||
|---|---|---|---|---|---|---|---|---|---|
| EPIC | Kp (mag) | HIP ID | EDR3 ID | Dist (pc) | RUWE | E(B – V) (mmag) | LSPC (L⊙) | LlRFM (L⊙) | Notes |
| 201623069 | 8.50 | 54281 | 3811534951212403072 |  |
1.28 | 10±16 | 5 43 ± 0 09 | 5.38 ± 0.08 | |
| 201644284 | 8.20 | 60264 | 3701419896778537216 | 90.2 ± 0.2 | 0.894 | 3.18 ± 0.05 | 3.22 ± 0.03 | ||
| 201725213 | 10.17 | 54262 | 3814827954178529664 |  |
1.203 | 23 ± 25 | 4.20 ± 0.10 | 4.22 ± 0.09 | |
| 203530127 | 7.11 | 82708 | 6034500386022688896 | 67.6 ± 0.1 | 0.882 | 4.72 ± 0.05 | 4.73 ± 0.04 | ||
| 211311380 | 9.13 | 41378 | 600698184764497664 | 105.6 ± 0.2 | 0.982 | 4±15 | 2.44 ± 0.03 | 2.42 ± 0.02 | K2-93, S(1,2,3) |
| 211388537(a) | 12.29 | 604703052788343296 |  |
0.909 | 41 ± 4(b) | 8.68 ± 0.40 | 8.62 ± 0.41 | S(4) | |
| 211401787 | 9.71 | 601159910928534144 |  |
1.059 | 9±16 | 2.95 ± 0.04 | 2.90 ± 0.04 | ||
| 211403248(a) | 12.31 | 604901823875341056 |  |
1.023 | 41 ± 4(b) | 8.04 ± 0.37 | 7.96 ± 0.35 | S(4) | |
| 211405262(a) | 12.66 | 604912647193030016 |  |
1.012 | 41 ± 4(b) | 6.43 ± 0.28 | 6.49 ± 0.27 | ||
| 211409088(a) | 12.82 | 604916770361557504 |  |
1.015 | 41 ± 4(b) | 5.38 ± 0.24 | 5.41 ± 0.23 | S(4) | |
Notes. The table is available in its entirety in the machine-readable format at the CDS. A portion is shown here for guidance regarding its form and content. The table provides identifiers and astrometric parameters for the 173 targets under study, sorted by EPIC ID. “Kp” gives the Kepler magnitude (Brown et al. 2011; Huber et al. 2016); “HIP ID” and “EDR3 ID” give the HIPPARCOS (Perryman et al. 1997) and Gaia EDR3 (Gaia Collaboration 2021) identifiers of the target; “Dist” gives the photogeometric distance from Bailer-Jones et al. (2021), unless otherwise stated; “RUWE” gives the renormalised unit weight error from Gaia (Lindegren et al. 2018); E(B – V) gives the reddening from the 3D dust maps for the Stilism project (Capitanio et al. 2017), unless otherwise stated. “LSPC” and “LIRFM” refer to luminosities calulated using Gaia EDR3 data combined with Teff and log 𝑔 from either SPC or IRFM (see Sect. 4.2). In the Notes column “RVEH” is short for radial velocity exoplanet host; “WDS” is short for Washington double star; “S” refers to a seismic investigation; the number in parenthesis refers to the reference listed in the table references listed below. (a)Member of M67; (b)M67 reddening from Taylor (2007);(c)Distance from Gaia DR2 (Bailer-Jones et al. 2018).
References. (1) Vanderburg et al. (2016); (2) Lund et al. (2019); (3) Bryant et al. (2021); (4) Stello et al. (2016); (5) Giguere et al. (2015); (6) Ment et al. (2018); (7) Grunblatt et al. (2019); (8) Washington Double Star Catalog (Mason et al. 2001); (9) Ong et al. (2021); (10) Pope et al. (2016); (11) Kruse et al. (2019); (12) Robinson et al. (2007); (13) North et al. (2017); (14) Pourbaix et al. (2004); (15) Griffin (2013); (16) Johnson et al. (2011); (17) Luhn et al. (2019); (18) Tamuz et al. (2008); (19) Moutou et al. (2011); (20) Ginski et al. (2016); (21) Van Eylen et al. (2018); (22) Jones et al. (2021).
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