Table D.1.
Subcluster probabilities for known members
| ID Gaia EDR3 | RA | DEC | ϖ ± ϖe | μα ± μαe | μδ ± μδe | RUWE | PA | PB | PC | PD | PE | PF | PG | Subcluster | Mem | Refs. |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (mas) | (mas/yr) | (mas/yr) | ||||||||||||
| 2178420537960651264 | 323.817830 | 57.472808 | 1.065±0.052 | -3.117±0.067 | -5.102±0.064 | 0.973 | 0.99 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.01 | A | Y | 2 |
| 2178434938995215232 | 323.827559 | 57.569180 | 1.101±0.032 | -2.990±0.039 | -4.903±0.036 | 1.060 | 1.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | A | Y | 2 |
| 2178434217440720512 | 323.852133 | 57.550292 | 1.180±0.058 | -3.065±0.070 | -4.882±0.061 | 0.968 | 1.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | A | Y | 2 |
| 2178417656046880384 | 323.957301 | 57.401123 | 1.142±0.051 | -4.139±0.066 | -5.210±0.060 | 1.020 | 0.01 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.99 | G | Y | 2 |
| 2178446174630143488 | 324.031103 | 57.574794 | 0.650±0.057 | -2.818±0.071 | -2.139±0.062 | 0.952 | 0.00 | 0.02 | 0.00 | 0.00 | 0.00 | 0.00 | 0.98 | G | Y | 11 |
| 2178391886229562624 | 324.614155 | 57.455895 | 1.414±0.301 | 0.208±0.738 | -2.928±0.494 | 1.206 | 0.10 | 0.06 | 0.00 | 0.00 | 0.41 | 0.00 | 0.43 | E/G | P2 | 2 |
| 2179201053771428480 | 323.106599 | 57.827847 | 1.153±0.086 | -3.981±0.099 | -4.161±0.092 | 1.033 | 0.00 | 0.00 | 0.00 | 0.00 | 0.00 | 0.01 | 0.01 | - | NS | 8 |
| 2178465759681247104 | 323.981837 | 57.844343 | 0.722±0.043 | -3.409±0.050 | -3.357±0.046 | 0.944 | 0.00 | 0.01 | 0.00 | 0.42 | 0.00 | 0.00 | 0.57 | D/G | P2 | 8 |
| 2178483072676684928 | 325.340837 | 57.681176 | 1.297±0.147 | -2.101±0.170 | -2.097±0.167 | 1.390 | 0.00 | 0.79 | 0.00 | 0.00 | 0.00 | 0.00 | 0.21 | B | P | 8 |
| 2178487681188556928 | 325.649571 | 57.747945 | 1.000±0.058 | -1.462±0.074 | -3.911±0.071 | 1.000 | 0.14 | 0.06 | 0.00 | 0.00 | 0.61 | 0.00 | 0.19 | E | P | 8 |
Notes. Column 1: ID Gaia EDR3. Columns 2, 3, 4, 5, and 6 are the astrometric parameters of each source, position, parallax, and proper motion, along with errors, respectively. Column 7: RUWE value. Columns 8 to 14 show the probability for each source belonging to one of the subclusters, A, B, C, D, E, F, and the extended population G. Column 15: Subcluster to which the source belongs. Column 16: Membership labeled as "Y" (member, with probability > 80%), "P" (probable member to belong to one of the subclusters, with probability < 80%), "P2" (probable member of belonging to two subclusters with probabilities > 40%), "NS" (no subcluster, low probability of not belonging to any cluster). Column 17: References of previous studies, (1) Sicilia-Aguilar et al. (2004); (2) Sicilia-Aguilar et al. (2005); (3) Sicilia-Aguilar et al. (2006a); (4) Mercer et al. (2009); (5) Morales-Calderón et al. (2009); (6) Barentsen et al. (2011); (7) Getman et al. (2012); (8) Nakano et al. (2012); (9) Rebull et al. (2013); (10) Sicilia-Aguilar et al. (2013); (11) Sicilia-Aguilar et al. (2015); (12) Meng et al. (2019). The complete version of 578 known members is available in electronic format via CDS.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.