Table 2.
Overview of fields in our final star catalogue.
| Source_id | x | y | z | vx | vy | vz |
|---|---|---|---|---|---|---|
| [km s−1] | [km s−1] | [km s−1] | ||||
| 494990686553088 | −0.82 | 0.07 | −0.92 | −252.3 | −249.5 | 29.7 |
| 2131751183780736 | −0.52 | 0.07 | −0.54 | −262.9 | −247.3 | 45.4 |
| 2412092288843648 | −0.12 | 0.01 | −0.12 | −105.8 | −210.9 | −51.9 |
| 4032119593003520 | −1.56 | 0.17 | −1.49 | 220.9 | −239.3 | 72.0 |
| 4564455019620096 | −0.58 | 0.09 | −0.66 | −204.4 | −83.7 | 57.1 |
| 4641558272441088 | −0.65 | 0.11 | −0.74 | 13.8 | −91.5 | −283.0 |
| 5201244050756096 | −0.76 | 0.12 | −0.81 | 127.5 | −120.1 | −201.5 |
| 5366583111858688 | −0.41 | 0.07 | −0.45 | 169.9 | −108.1 | −93.3 |
| 6932768706211328 | −1.58 | 0.22 | −1.55 | 176.6 | −253.7 | 99.5 |
| 7299795136273664 | −0.74 | 0.13 | −0.72 | 273.0 | −256.0 | 95.1 |
| E | L⊥ | Lz | Significance | Labelorig | LabelDcut | D |
| [105 km2 s−2] | [103 kpc km s−1] | [103 kpc km s−1] | ||||
| −1.192 | 0.56 | −0.06 | 8.9 | 24 | 24 | 1.43 |
| −1.184 | 0.60 | −0.04 | 8.9 | 24 | 24 | 1.16 |
| −1.485 | 0.36 | 0.28 | 6.3 | 3 | 3 | 1.46 |
| −1.141e | 0.43 | 0.10 | 5.5 | 26 | 0 | 2.27 |
| −1.172 | 0.70 | 1.40 | 3.4 | 30 | 30 | 1.34 |
| −1.002 | 2.46 | 1.36 | 9.8 | 60 | 60 | 1.79 |
| −1.133 | 1.85 | 1.14 | 3.6 | 61 | 61 | 1.76 |
| −1.228 | 0.83 | 1.19 | 3.1 | 38 | 38 | 1.61 |
| −1.206 | 0.75 | −0.04 | 8.9 | 24 | 24 | 0.83 |
| −1.042 | 0.71 | −0.06 | 3.6 | 51 | 51 | 1.63 |
Notes. It contains Gaia source ids, heliocentric Cartesian coordinates, heliocentric Cartesian velocities, and the three features we used for clustering. The column significance indicates the significance of the cluster to which a star belongs (according to the original single−linkage assignment), Labelorig is the label of the cluster according to the single-linkage process, and LabelDcut is the cluster label after selecting the cluster with the smallest Mahalanobis distance D (requiring at least D < 2.13). The full table is made available at the CDS.
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