Table B.3
Gaia DR3 (Gaia Collaboration 2023) parallax (ϖ), goodness-of-fit (GOF), and RUWE of target stars. The geometric distances from Bailer-Jones et al. (2021) are listed and adopted for the calculations in this work. The calculated vertical distances from the Galactic disk are also included in the Table. The last column contains the subclass of each target.
Name | ϖ [mas] | ϖ/σϖ | RUWEa | GOFb | Dist. (B-J) [kpc] | z [kpc] | Subclass |
---|---|---|---|---|---|---|---|
WR-C-01 | 0.131±0.014 | 9.4 | 1.06 | 1.96 | ![]() |
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WN4 |
WR-C-02 | 0.261±0.016 | 16.0 | 1.03 | 0.62 | ![]() |
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Not WR |
WR-C-03 | 0.105±0.042 | 2.5 | 1.08 | 1.74 | ![]() |
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Not WR |
WR-C-04 | 0.137±0.041 | 3.4 | 0.98 | −0.54 | ![]() |
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.. |
WR-C-05 | −0.155±0.067 | − | 3.86 | 53.56 | ![]() |
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WC5 |
WR-C-06 | 0.147±0.024 | 6.0 | 1.05 | 1.26 | ![]() |
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Not WR |
WR-C-07 | 0.029±0.045 | 0.6 | 1.20 | 5.69 | ![]() |
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.. |
WR-C-08 | 0.161±0.082 | 2.0 | 1.21 | 5.25 | ![]() |
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.. |
WR-C-09 | 0.114±0.040 | 2.9 | 1.01 | 0.33 | ![]() |
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.. |
WR-C-10 | 0.156±0.022 | 7.3 | 1.20 | 5.21 | ![]() |
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WC5+abs |
WR-C-11 | 0.056±0.019 | 2.9 | 0.98 | −0.56 | ![]() |
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WN5 |
WR-C-12 | 0.196±0.049 | 4.0 | 0.99 | −0.25 | ![]() |
![]() |
.. |
WR-C-13 | 0.224±0.074 | 3.0 | 1.01 | 0.36 | ![]() |
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.. |
WR-C-14 | 0.258±0.023 | 11.2 | 1.76 | 22.87 | ![]() |
![]() |
WC9 |
WR-C-15 | −0.022±0.083 | − | 1.00 | 0.11 | ![]() |
![]() |
.. |
WR-C-16 | 0.099±0.043 | 2.3 | 1.17 | 5.13 | ![]() |
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WC8 |
WR-C-17 | −0.062±0.056 | − | 1.05 | 1.32 | ![]() |
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.. |
WR-C-18 | 0.193±0.054 | 3.6 | 1.12 | 3.22 | ![]() |
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WC9d |
WR-C-19 | 0.037±0.050 | 0.7 | 1.01 | 0.40 | ![]() |
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.. |
WR-C-20 | 1.954±0.188 | 10.4 | 2.84 | 45.67 | ![]() |
![]() |
.. |
WR-C-21 | 0.144±0.029 | 5.0 | 1.07 | 1.86 | ![]() |
![]() |
WC7 |
WR-C-22 | 0.075±0.109 | 0.7 | 1.23 | 6.17 | ![]() |
![]() |
.. |
WR-C-23 | 0.203±0.018 | 11.5 | 1.03 | 0.79 | ![]() |
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WN8 |
WR-C-24 | 0.180±0.053 | 3.4 | 1.09 | 2.74 | ![]() |
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WC9d |
WR-C-25 | 0.165±0.129 | 1.3 | 1.09 | 2.11 | ![]() |
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.. |
WR-C-26 | 0.413±0.021 | 19.4 | 0.92 | −1.57 | ![]() |
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WN6 |
WR-C-27 | 0.090±0.049 | 1.8 | 0.98 | −0.43 | ![]() |
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.. |
WR-C-28 | 0.272±0.018 | 14.9 | 1.08 | 1.92 | ![]() |
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WN6+abs |
WR-C-29 | 0.395±0.018 | 21.5 | 0.87 | −2.87 | ![]() |
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WN7 |
WR-C-30 | −0.135±0.133 | − | 1.09 | 2.90 | ![]() |
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.. |
WR-C-31 | 0.124±0.028 | 4.4 | 1.06 | 1.46 | ![]() |
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WC8 |
WR-C-32 | 0.240±0.030 | 7.9 | 0.89 | −2.33 | ![]() |
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WC9d |
WR-C-33 | 0.120±0.077 | 1.6 | 0.96 | −0.78 | ![]() |
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.. |
WR-C-34 | 0.253±0.072 | 3.5 | 1.09 | 1.75 | ![]() |
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.. |
WR-C-35 | 0.171±0.027 | 6.4 | 1.12 | 2.46 | ![]() |
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WN8 |
WR-C-36 | 0.297±0.025 | 11.8 | 1.05 | 1.08 | ![]() |
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WN7h |
WR-C-37 | 0.116±0.045 | 2.6 | 1.08 | 1.63 | ![]() |
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WC9 |
WR-C-38 | 0.179±0.043 | 4.2 | 0.91 | −1.91 | ![]() |
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WC9 |
WR-C-39 | 0.128±0.028 | 4.6 | 1.02 | 0.50 | ![]() |
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WN7-8 |
WR-C-40 | 0.211±0.064 | 3.3 | 3.18 | 36.63 | ![]() |
![]() |
WC9 |
WR-C-41 | 0.045±0.040 | 1.1 | 0.99 | −0.26 | ![]() |
![]() |
WN5-6 |
WR-C-42 | 0.035±0.035 | 1.0 | 1.06 | 1.19 | ![]() |
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WN6 |
WR-C-43 | 0.199±0.053 | 3.8 | 1.15 | 3.14 | ![]() |
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WC9d |
WR-C-44 | 0.165±0.037 | 4.5 | 1.09 | 1.84 | ![]() |
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WN5-6 |
WR-C-45 | 0.182±0.108 | 1.7 | 1.12 | 2.46 | ![]() |
![]() |
.. |
WR-C-46 | 0.242±0.031 | 7.8 | 1.32 | 5.77 | ![]() |
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WC8 |
WR-C-47 | 0.140±0.048 | 2.9 | 1.10 | 2.36 | ![]() |
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WC6 |
WR-C-48 | −1.902±0.452 | − | 13.84 | 251.32 | ![]() |
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WC7 |
WR-C-49 | − | − | − | 669.89 | − | − | .. |
WR-C-50 | 0.206±0.142 | 1.4 | 9.60 | 162.57 | ![]() |
![]() |
WN5-6 |
WR-C-51 | −0.077±0.083 | − | 0.92 | −3.11 | ![]() |
![]() |
.. |
WR-C-52 | 0.101±0.047 | 2.2 | 1.03 | 0.87 | ![]() |
![]() |
.. |
WR-C-53 | 0.122±0.045 | 2.7 | 0.98 | −0.53 | ![]() |
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.. |
WR-C-54 | 0.271±0.015 | 17.7 | 1.43 | 11.72 | ![]() |
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WN6+abs |
WR-C-55 | 0.099±0.023 | 4.2 | 1.04 | 1.05 | ![]() |
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WN3 |
WR-C-56 | −0.051±0.078 | − | 1.07 | 1.78 | ![]() |
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.. |
WR-C-57 | 0.114±0.028 | 4.0 | 1.07 | 2.06 | ![]() |
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WN/C |
WR-C-58 | 0.126±0.025 | 5.0 | 1.15 | 3.80 | ![]() |
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WC5 |
WR-C-59 | 0.084±0.023 | 3.7 | 1.00 | −0.01 | ![]() |
![]() |
WN3 |
Notes. aRenormalized unit weight error (RUWE). A value close to 1.0 suggests a good fit with a single-star model, whereas notably higher values may point to problems with the astrometric solution or the presence of a binary companion. bGoodness-of-fit statistic for the astrometric solution. As per the Gaia DR3 documentation, values of ≳3 indicate a poor fit to the observed data.
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