Table 2
Stars in our sample classified by BANYAN Σ with a high Bayesian probability of belonging to a young stellar association.
| Karmn | Name(a) | BANYAN Σ Prob.(b) | Young association(c) | Association reference |
|---|---|---|---|---|
| J02088+494 | G 173−039 | 99.94% | AB Doradus | Zuckerman et al. (2004) |
| J02519+224 | RBS 365 | 99.79% | β Pictoris | Zuckerman et al. (2001) |
| J03473−019 | G 080−021 | 99.94% | AB Doradus | Zuckerman et al. (2004) |
| J05019+011(d) | 1RXS J050156.7+010845 | 99.91% | β Pictoris | Zuckerman et al. (2001) |
| J05062+046(d) | RX J0506.2+0439 | 99.79% | β Pictoris | Zuckerman et al. (2001) |
| J09163−186 | LP 787−052 | 95.01% | Argus | Zuckerman (2018) |
| J10289+008 | BD+01 2447 | 99.97% | AB Doradus | Zuckerman et al. (2004) |
| J19511+464 | G 208−042 | 94.17% | Argus | Zuckerman (2018) |
| J21164+025 | LSPM J2116+0234 | 85.20% | Argus | Zuckerman (2018) |
Notes. (a)As in Cifuentes et al. (2020). (b)The Bayesian probability that this object belongs to the young stellar association. (c)Most probable Bayesian hypothesis (including the field).(d) Already mentioned in Schw19 as candidate members of the corresponding young stellar association.
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