Table D.1.
Properties of the 634 candidate members.
| source_id | Group | mem_prob | ra | dec | mean_X | sd_X | mean_Y | sd_Y | mean_Z | sd_Z | mean_U | sd_U | mean_V | sd_V | mean_W | sd_W | lower_Mass | map_Mass | upper_Mass | lower_Av | map_Av | upper_Av |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| - | - | - | deg | deg | [pc] | [pc] | [pc] | [pc] | [pc] | [pc] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | [M⊙] | [M⊙] | [M⊙] | - | - | - |
| 1512001425052135680 | Latyshev_2 | 1.000 | 212.692 | 52.021 | -49.460 | 0.166 | -31.743 | 0.108 | 75.281 | 0.229 | -3.045 | 0.281 | 7.478 | 0.179 | -4.883 | 0.424 | 0.269 | 0.278 | 0.290 | 0.021 | 0.096 | 0.087 |
| 1405053814507528832 | Mecayotl_1 | 1.000 | 239.061 | 53.250 | -32.918 | 0.418 | -54.925 | 0.714 | 85.742 | 1.061 | -2.803 | 0.389 | 7.009 | 0.623 | -7.537 | 0.982 | 0.132 | 0.136 | 0.139 | 0.018 | 0.051 | 0.088 |
| 1559650754307292544 | Latyshev_2 | 1.000 | 203.036 | 51.872 | -52.115 | 1.256 | -22.226 | 0.637 | 72.393 | 1.742 | -2.901 | 0.417 | 7.532 | 0.214 | -4.886 | 0.482 | 0.359 | 0.370 | 0.379 | 0.016 | 0.068 | 0.085 |
| 1669197262444734976 | Mecayotl_1 | 1.000 | 223.262 | 65.723 | -31.321 | 0.649 | -29.474 | 0.634 | 95.329 | 2.042 | -4.309 | 0.396 | 7.036 | 0.399 | -7.542 | 1.126 | 0.236 | 0.251 | 0.267 | 0.016 | 0.080 | 0.087 |
| 1483407937977056384 | ComaBer_tails | 1.000 | 210.965 | 36.378 | -59.826 | 0.384 | -35.899 | 0.234 | 51.399 | 0.331 | -1.831 | 0.265 | 3.314 | 0.156 | -3.891 | 0.224 | 0.158 | 0.161 | 0.165 | 0.019 | 0.079 | 0.087 |
| 1459368662422928384 | ComaBer_tails | 1.000 | 197.925 | 25.963 | -72.689 | 0.181 | -23.513 | 0.065 | 37.199 | 0.091 | -2.447 | 0.083 | 4.004 | 0.030 | -3.042 | 0.043 | 0.730 | 0.738 | 0.744 | 0.018 | 0.063 | 0.086 |
| 1598228528516035200 | Mecayotl_1 | 1.000 | 236.477 | 54.692 | -35.106 | 0.084 | -52.993 | 0.133 | 89.755 | 0.230 | -3.462 | 0.376 | 6.844 | 0.568 | -7.046 | 0.961 | 0.401 | 0.411 | 0.422 | 0.023 | 0.078 | 0.088 |
| 4008390933229933184 | ComaBer_core | 1.000 | 186.910 | 25.912 | -75.475 | 0.203 | -9.146 | 0.036 | 36.938 | 0.111 | -2.388 | 0.534 | 4.678 | 0.068 | -3.139 | 0.262 | 0.320 | 1.729 | 1.736 | 0.020 | 0.080 | 0.087 |
| 1597061946678694016 | Mecayotl_1 | 1.000 | 236.059 | 53.874 | -35.274 | 0.242 | -52.416 | 0.363 | 86.551 | 0.544 | -2.852 | 0.414 | 7.015 | 0.611 | -7.320 | 1.009 | 0.174 | 0.177 | 0.182 | 0.019 | 0.074 | 0.087 |
| 1560767995559564032 | Latyshev_2 | 1.000 | 207.493 | 53.246 | -49.202 | 0.086 | -25.605 | 0.046 | 74.269 | 0.127 | -2.648 | 0.054 | 7.626 | 0.031 | -5.001 | 0.079 | 0.476 | 0.485 | 0.495 | 0.024 | 0.070 | 0.088 |
Notes. This table will be available in its entirety in machine-readable form at the CDS. For each candidate member, we provide its Gaia DR3 source id, parent group, sky coordinates, mean and standard deviation of the Cartesian ICRS phase-space coordinates X, Y, Z, U, V, and W, and lower percentiles (2.5%), maximum-a-posteriori, and upper percentiles (97.5%) of the estimated mass and extinction in the V band.
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