Table B.4
Absolute Mv magnitudes of selected WR candidates. The distances from Bailer-Jones et al. (2021) were used in all the calculations (see Table B.3).
| Name | v [mag] | (b − v)a [mag] | (b − v)b [mag] |  [mag] |
 [mag] |
 [mag] |
 [mag] |
Subclass |
|---|---|---|---|---|---|---|---|---|
| WR-C-01 | 14.96±0.01 | 1.08±0.03 | 1.30±0.11 | 5.8±0.4 | 6.7±0.6 | −4.7±0.5 | −5.7±0.6 | WN4 |
| WR-C-02 | 11.43±0.02 | 0.57±0.03 | 0.38±0.02 | av 3.6±0.4 | av 2.8±0.4 | −4.9±0.5 | −4.1±0.4 | Not WR |
| WR-C-03 | 16.34±0.02 | 0.63±0.05 | − | av 3.8±0.5 | − | −1.6±0.7 | − | Not WR |
| WR-C-05 | 16.57±0 .07 | 1.60±0.17 | − | 7.4±1.1 | − | −6.2±1.2 | − | WC5 |
| WR-C-06 | 17.22±0 .04 | 1.46±0.15 | − | av 7.3±0.7 | − | −3.5±0.8 | − | Not WR |
| WR-C-10 | 16.88±0 11 | 1.27±0.35 | − | 6.1±1.7 | − | −2.7±1.7 | − | WC5+abs |
| WR-C-11 | 15.86±0 .02 | 1.03±0.05 | − | 5.4±0.5 | − | −4.6±0.6 | − | WN5 |
| WR-C-14 | 15.59±0 .02 | 1.22±0.06 | 0.90±0.14 | 6.4±0.5 | 5.0±0.7 | −3.3±0.5 | −2.0±0.7 | WC9 |
| WR-C-15 | 20.49±0.27 | 2.33:: | av 10.9:: | −4.3::† | .. | |||
| WR-C-16 | 18.96±0.10 | 1.54±0.47 | − | 7.9±2.0 | − | −3.0±2.1 | − | WC8 |
| WR-C-18 | 19.34±0.18 | 4.02:: | − | 17.9:: | − | −11.4::† | − | WC9d |
| WR-C-19 | 19.46±0.12 | 2.99:: | − | av 13.6:: | − | −8.7::† | − | .. |
| WR-C-20 | 21.01 ±0.67 | 0.96:: | − | av 5.2:: | − | 7.3::† | − | .. |
| WR-C-21 | 17.63±0.09 | 1.48±0.29 | − | 6.9±1.4 | − | −2.8±1.5 | − | WC7 |
| WR-C-23 | 15.47±0.02 | 1.56±0.07 | 1.32±0.08 | 7.0±0.5 | 6.1±0.5 | −4.5±0.5 | −3.6±0.5 | WN8 |
| WR-C-24 | 19.47±0.15 | 2.40:: | − | 11.2:: | − | −4.8::† | − | WC9d |
| WR-C-25 | 21.58±0.96 | −0.24:: | − | av 0.2:: | − | 7.5::† | − | .. |
| WR-C-26 | 12.24±0.01 | 0.72±0.03 | 0.73±0.01 | 4.1±0.4 | 4.1±0.4 | −3.7±0.4 | −3.7±0.4 | WN6 |
| WR-C-27 | 19.74±0.22 | 2.93:: | av 13.3:: | −7.5::† | .. | |||
| WR-C-28 | 11.99±0.01 | 1.02±0.01 | 0.99±0.02 | 5.4±0.4 | 5.2±0.4 | −5.9±0.4 | −5.8±0.4 | WN6+abs |
| WR-C-29 | 12.60±0.01 | 0.88±0.02 | 0.89±0.02 | 4.3±0.4 | 4.3±0.4 | −3.5±0.4 | −3.6±0.4 | WN7 |
| WR-C-31 | 18.81±0.19 | 1.44±0.56 | − | 7.5±2.4 | − | −2.3±2.4 | − | WC8 |
| WR-C-32 | 14.86±0.03 | 1.42±0.07 | 0.92±0.25 | 7.2±0.5 | 5.1±1.1 | −5.3±0.6 | −3.3±1.2 | WC9d |
| WR-C-35 | 16.69±0.05 | 1.81±0.21 | 8.1±0.9 | −4.5±1.0 | WN8 | |||
| WR-C-36 | 15.65±0.03 | 1.13±0.08 | − | 5.3±0.5 | − | −2.0±0.5 | − | WN7h |
| WR-C-38 | 19.07±0.19 | 1.43±0.70 | − | 7.2±2.9 | − | −1.3±2.9 | − | WC9 |
| WR-C-39 | 17.30±0.06 | 1.53±0.28 | − | 6.9±1.2 | − | −3.3±1.3 | − | WN7-8 |
| WR-C-40 | 15.27±0.06 | 1.47±0.40 | 1.59±0.13 | 7.4±1.7 | 7.9±0.7 | −5.3±1.8 | −5.8±0.9 | WC9 |
| WR-C-43 | 19.81 ±0.30 | 2.12:: | 10.1:: | −3.0::† | WC9d | |||
| WR-C-44 | 17.83±0.07 | 2.40±0.68 | − | 11.0±2.8 | − | −6.8±2.9 | − | WN5-6 |
| WR-C-48 | 18.50±0.09 | 1.44±0.36 | − | 6.8±1.7 | − | −2.1±1.8 | − | WC7 |
| WR-C-49 | 17.29±0.03 | 0.48±0.08 | − | av 3.2±0.5 | − | − | − | .. |
| WR-C-50 | 15.77±0.04 | 1.61±0.10 | 1.60±0.25 | 7.8±0.6 | 7.8±1.1 | −5.3±1.0 | −5.3±1.4 | WN5-6 |
| WR-C-52 | 18.68±0.06 | 2.05±0.57 | av 9.7±2.4 | −5.2±2.4 | .. | |||
| WR-C-54 | 11.20±0.01 | 0.90±0.02 | 0.91±0.02 | 4.8±0.4 | 4.9±0.4 | −6.3±0.4 | −6.3±0.4 | WN6+abs |
| WR-C-55 | 17.40±0.04 | 1.42±0.12 | 7.2±0.6 | −4.0±0.7 | WN3 | |||
| WR-C-57 | 18.65±0.09 | 1.79±0.54 | − | 8.3±2.3 | − | −3.6±2.3 | − | WN/C |
| WR-C-58 | 18.35±0.12 | 2.88:: | − | 12.7:: | − | −8.1::† | − | WC5 |
| WR-C-59 | 16.02±0.02 | 0.82±0.04 | − | 4.7±0.4 | − | −3.4±0.6 | − | WN3 |
Notes. aDerived from Gaia XP spectra. bDerived from our spectra for objects with (G < 14 mag).av The average WR intrinsic color was adopted for calculation as the actual WR subtype is not available (targets not observed in this work or classified as non-WR). †Candidates with error on Mv greater than 4 mag and not included in Fig.11.
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