Table E.1.
New members found from the Mahalanobis distance analysis, using the Gaia EDR3
| ID Gaia EDR3 | RA | DEC | ϖ ± ϖe | μα ± μαe | μδ ± μδe | RUWE | PA | PB | PE | PF | Subcluster |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (mas) | (mas/yr) | (mas/yr) | |||||||
| 2203402614670559232 | 326.063135 | 59.360206 | 1.112 ± 0.016 | -2.230 ± 0.019 | -4.181 ± 0.016 | 0.975 | 0.95 | —- | —- | —- | A |
| 2203398697660400768 | 326.168794 | 59.323927 | 1.069 ± 0.031 | -2.507 ± 0.038 | -4.368 ± 0.030 | 1.027 | 0.95 | —- | —- | —- | A |
| 2203412888232208640 | 325.827953 | 59.366154 | 1.123 ± 0.013 | -2.880 ± 0.015 | -2.966 ± 0.014 | 1.094 | —- | 0.95 | —- | —- | B |
| 2203406188083035776 | 325.664257 | 59.244763 | 1.046 ± 0.015 | -2.560 ± 0.017 | -2.837 ± 0.015 | 1.169 | —- | 0.95 | —- | —- | B |
| 2202645188605787648 | 326.367554 | 59.141696 | 1.084 ± 0.055 | -1.320 ± 0.069 | -3.031 ± 0.060 | 1.232 | —- | —- | 0.95 | —- | E |
| 2203405565302940416 | 325.580452 | 59.249619 | 1.112 ± 0.011 | -1.309 ± 0.013 | -3.185 ± 0.011 | 0.906 | —- | —- | 0.95 | —- | E |
| 2179429344178082048 | 324.761669 | 59.134190 | 1.042 ± 0.039 | -3.645 ± 0.047 | -3.731 ± 0.052 | 0.988 | —- | —- | —- | 0.95 | F |
| 2178408683842112896 | 323.753814 | 57.204424 | 1.160 ± 0.017 | -3.513 ± 0.019 | -3.944 ± 0.018 | 1.114 | —- | —- | —- | 0.95 | F |
| 2178328355081854976 | 326.554329 | 57.902130 | 1.104 ± 0.080 | -1.558 ± 0.087 | -3.230 ± 0.090 | 0.998 | —- | 0.34 | 0.61 | —- | B/E |
| 2179397355261072768 | 324.037597 | 58.792397 | 1.095 ± 0.030 | -1.543 ± 0.034 | -3.209 ± 0.034 | 1.055 | —- | 0.38 | 0.57 | —- | B/E |
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 their errors. Column 7: RUWE value. Columns 8 to 11 show the probability for each source belonging to one of the subclusters, or in some cases, to two subclusters. Column 12: The subcluster to which the source belongs. The complete version of 334 new members is available in electronic format via CDS.
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