Table A.1
Membership of target stars in nearby young associations.
| Target name | Group | Pmemb | Refs. | SigMA cluster |
|---|---|---|---|---|
| HD 31305 | TAU | 81.1 | 1,2,9,10 | . . . |
| HD 112532 | LCC | 99.4 | 5 | σ Cen |
| HD 131960 | UCL | 90.0 | 8 | Libra-South |
| HD 141960 | US | 63.1 | 3,6,7 | ρ Sco |
| HD 144277 | UCL | 99.9 | 3,6 | η Lup |
| HD 145101 | US | 99.9 | 6,7 | δ Sco |
| HD 152989 | UCL | 93.6 | 8 | η Lup |
| HD 155853 | UCL | 71.5 | . . . | Scorpio-Body |
| HD 176497 | UCRA | 100.0 | 3,4 | CrA-North |
Notes. Column 2 and 3 summarize the outcomes of BANYAN Σ, showing the most probable young association to which the star may belong (Col. 2) and the obtained membership probability (Col. 3). Column 4 lists references for previous studies dealing with the star’s membership in the respective group. Using a novel clustering method (SigMA) and harnessing the unique potential of Gaia DR3, Ratzenböck et al. (2023b) proposed a new division of young stars in the Sco-Cen region. Column 5 shows the names of the subgroups to which the stars belong in this new classification. References used in this table: (1): Cody et al. (2013); (2): Gagné et al. (2018); (3): Gagné & Faherty (2018); (4): Galli et al. (2020); (5): Goldman et al. (2018); (6): Hoogerwerf (2000); (7): Luhman et al. (2018); (8): Luhman (2022); (9): Luhman (2023); (10): Mooley et al. (2013).
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