Table 4
Membership classification of the TITANS.
| Star | Parallax (mas) | vhelio (km s−1) | Membership |
|---|---|---|---|
| BD+24 1676 | 3.964 ± 0.017 | − 237.48 ± 0.95 | GE †‡ |
| BD − 10 388 | 4.229 ± 0.024 | 36.79 ± 0.86 | – |
| BPS CS22166-030 | 0.842 ± 0.010 | 92.0 ± 2.4 | GE† |
| CD − 33 3337§ | 8.173 ± 0.016 | 73.79 ± 0.25 | HS† |
| CD − 35 14849 | 6.296 ± 0.034 | 108.18 ± 0.92 | GE†/Sq‡ |
| HD 16031 | 8.230 ± 0.016 | 24.72 ± 0.39 | – |
| HD 166913 | 16.707 ± 0.029 | − 48.61 ± 0.30 | – |
| HD 218502 | 13.374 ± 0.038 | − 29.48 ± 0.48 | – |
| HD 34328§ | 13.759 ± 0.010 | 235.25 ± 0.28 | Sq †‡ |
| HD 59392 | 6.382 ± 0.013 | 268.42 ± 0.33 | GE†/Sq‡ |
| BD + 02 4651§ | 5.595 ± 0.020 | − 251.11 ± 0.38 | GE†/Sq‡ |
| BD+03 740 | 5.893 ± 0.026 | 174.5 ± 1.6 | GE† |
| BD − 13 3442 | 4.703 ± 0.031 | 116.1 ± 1.5 | GE† |
| BD+26 2621 | 4.804 ± 0.018 | − 62.2 ± 1.3 | GE†/Sq‡ |
| BD+26 4251 | 7.595 ± 0.016 | − 93.89 ± 0.23 | – |
| BD+29 2091 | 11.371 ± 0.019 | 83.23 ± 0.36 | GE† |
| CD − 30 18140 | 6.897 ± 0.023 | 17.91 ± 0.49 | GE† |
| CD − 33 1173 | 4.558 ± 0.016 | 47.7 ± 1.9 | GE† |
| CD − 48 2445§ | 5.369 ± 0.014 | 319.56 ± 0.60 | GE† |
| CD − 71 1234 | 6.110 ± 0.029 | 235.4 ± 1.0 | GE† |
| G 24 − 3 | 7.648 ± 0.020 | − 208.18 ± 0.29 | GE† |
| HD 108177 | 9.405 ± 0.018 | 155.31 ± 0.37 | GE† |
| HD 116064§ | 14.40 ± 0.14 | 143.70 ± 0.52 | GE† |
| HD 122196§ | 9.635 ± 0.034 | − 27.78 ± 0.38 | – |
| HD 126681 | 17.816 ± 0.023 | 45.40 ± 0.13 | – |
| HD 132475 | 10.671 ± 0.025 | 176.67 ± 0.22 | Sq‡ |
| HD 160617 | 9.525 ± 0.021 | 100.65 ± 0.35 | GE† |
| HD 189558 | 15.765 ± 0.024 | − 12.77 ± 0.14 | – |
| HD 193901 | 20.854 ± 0.023 | − 171.43 ± 0.14 | GE† |
| HD 213657 | 6.967 ± 0.016 | 51.82 ± 0.49 | – |
| HD 241253 | 10.068 ± 0.016 | − 15.91 ± 0.16 | – |
| HD 284248 | 11.378 ± 0.019 | 339.13 ± 0.36 | – |
| HD 74000 | 9.081 ± 0.017 | 206.17 ± 0.55 | GE† |
| HD 94028 | 20.208 ± 0.026 | 66.00 ± 0.25 | – |
| HE 0926 − 0508 | 2.190 ± 0.061 | 189.6 ± 1.6 | GE †‡ |
| LP 815 − 43 | 4.156 ± 0.018 | − 4.1 ± 1.6 | GE †‡ |
| LP 831 − 70 | 4.162 ± 0.022 | − 47.6 ± 1.7 | – |
| Ross 453 | 5.619 ± 0.020 | 99.14 ± 0.54 | Sq‡ |
| Ross 892 | 6.056 ± 0.018 | 88.53 ± 0.18 | GE† |
| UCAC2 20056019 | 1.017 ± 0.017 | − 7.69 ± 1.7 | GE† |
| Wolf 1492 | 3.649 ± 0.028 | 449.8 ± 3.4 | Sq† |
| HD 140283 | 16.267 ± 0.026 | − 170.37 ± 0.15 | GE† |
| HD 84937 | 13.500 ± 0.044 | − 15.69 ± 0.43 | GE† |
| HD 22879 | 38.325 ± 0.031 | 120.54 ± 0.21 | – |
| HD 298986 | 7.489 ± 0.012 | 198.21 ± 0.27 | HS† |
| HD 106038 | 7.449 ± 0.030 | 99.52 ± 0.26 | GE†/Sq‡ |
| HD 201891 | 29.877 ± 0.020 | − 44.15 ± 0.19 | – |
| HD 102200 | 13.861 ± 0.014 | 161.44 ± 0.27 | – |
Notes. The symbol §, following the star name, indicates a binary system identified in Kervella et al. (2019) or Hansen et al. (2017). Parallax values are from the Gaia EDR3 catalogue. In the membership column, GE means Gaia-Enceladus, HS Helmi streams, and Sq Sequoia (see Sect. 5). The symbol † means a likely membership according to the criterion of Massari et al. (2019) and ‡ means according to the criterion of Myeong et al. (2019). The bottom part of the table incorporates the metal-poor Gaia benchmark stars.
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