Table A.1.
Properties of OCs with at least one associated WD candidate as listed in Table 3.
| OC | ϖgr | AV | log t | [Fe/H] |
|---|---|---|---|---|
| (μa s) | (mag) | (yr) | (dex) | |
| Alessi 22 | 2821.6±9.8 | 0.3±0.13 | 8.8±0.2 | 0.0±0.0 |
| Alessi 62 | 1643.6±9.9 | 0.85±0.07 | 9.0±0.0 | 0.1±0.07 |
| Alessi 94 | 1811.7±9.7 | 0.12±0.08 | 8.3±0.2 | 0.0±0.0 |
| CWNU 41 | 1371.9±10.1 | 0.15±0.1 | 8.8±0.2 | 0.0±0.0 |
| HSC 1155 | 3536.1±9.6 | 0.16±0.11 | 8.3±0.3 | 0.0±0.0 |
| HSC 2304 | 934.3±10.3 | 0.2±0.11 | 8.3±0.2 | 0.0±0.0 |
| HSC 381 | 3199.8±8.7 | 0.21±0.15 | 7.5±0.3 | 0.0±0.0 |
| Mamajek 4 | 2251.5±8.7 | 0.21±0.03 | 8.8±0.0 | 0.05±0.08 |
| NGC 1901 | 2405.6±9.1 | 0.11±0.06 | 8.9±0.0 | -0.04±0.08 |
| NGC 2358 | 1107.6±10.2 | 0.37±0.07 | 8.8±0.1 | -0.01±0.09 |
| NGC 2516 | 2455.3±9.0 | 0.45±0.05 | 8.4±0.1 | -0.01±0.03 |
| NGC 3532 | 2119.3±9.2 | 0.14±0.02 | 8.6±0.0 | 0.05±0.03 |
| NGC 6633 | 2561.7±9.5 | 0.77±0.11 | 8.8±0.0 | -0.09±0.06 |
| NGC 752 | 2303.4±9.2 | 0.16±0.07 | 9.2±0.0 | -0.04±0.05 |
| Ruprecht 147 | 3293.3±9.4 | 0.29±0.05 | 9.5±0.0 | 0.09±0.05 |
| Stock 2 | 2706.3±8.7 | 0.79±0.06 | 8.9±0.1 | 0.03±0.05 |
| Theia 248 | 2087.1±9.1 | 0.61±0.18 | 8.0±0.2 | 0.0±0.0 |
| Theia 558 | 1462.9±9.7 | 0.65±0.19 | 8.3±0.2 | 0.0±0.0 |
| Theia 817 | 2799.2±9.2 | 0.25±0.16 | 8.3±0.3 | 0.0±0.0 |
| Turner 5 | 2418.4±9.2 | 0.23±0.06 | 8.6±0.1 | -0.08±0.04 |
| UPK 5 | 1812.8±9.7 | 0.74±0.06 | 8.0±0.2 | 0.02±0.05 |
Notes. OC group parallaxes (ϖgr) were computed according to the procedure in Maíz Apellániz et al. (2021). OC extinctions (AV), total ages (log t), and ([Fe/H]) were taken from Cantat-Gaudin et al. (2020), Dias et al. (2021), Hunt & Reffert (2023).
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