Table 6.
Gaia DR2 astrometric data for nine components of the [KPS2012] MWSC 3335 cluster (not including HD 194 649 A,B, for which no Gaia DR2 parallax or proper motions are available) with compatible parallaxes and proper motions and their aggregate results.
| Gaia DR2 ID | ϖ | μα* | μδ |
|---|---|---|---|
| (mas) | (mas/a) | (mas/a) | |
| 2067482773947102208 | 0.6009 ± 0.0269 | −3.140 ± 0.045 | −4.242 ± 0.041 |
| 2067483044525974784 | 0.6250 ± 0.0308 | −3.211 ± 0.053 | −4.134 ± 0.045 |
| 2067482602148428288 | 0.5542 ± 0.0264 | −3.166 ± 0.043 | −4.118 ± 0.043 |
| 2067482705227636480 | 0.5593 ± 0.0240 | −3.142 ± 0.039 | −4.180 ± 0.036 |
| 2067482945745805312 | 0.5753 ± 0.0168 | −3.300 ± 0.027 | −4.409 ± 0.029 |
| 2067482735291629056 | 0.6065 ± 0.0245 | −3.445 ± 0.034 | −3.811 ± 0.048 |
| 2067482877026323712 | 0.5757 ± 0.0189 | −2.890 ± 0.035 | −4.450 ± 0.029 |
| 2067482670867892352 | 0.5944 ± 0.0194 | −3.254 ± 0.035 | −4.293 ± 0.029 |
| 2067482945745805440 | 0.5826 ± 0.0230 | −3.040 ± 0.039 | −4.181 ± 0.034 |
| 0.5852 ± 0.0413 | −3.177 ± 0.065 | −4.036 ± 0.065 | |
Notes. The aggregate results use external uncertainties and include the spatial covariance terms of Lindegren et al. (2018).
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