Table E.1
Estimates of the cluster extinction using the sample mean ⟨AG⟩ (which is biased) and the maximum likelihood (ML) estimates of μ, as well as the global uncertainty σ.
| No. of | ML estimates | |||
|---|---|---|---|---|
| Name | stars | ⟨AG ⟩ |  |
 |
| mag | mag | mag | ||
| NGC3532 | 1217 | 0.293 |  |
 |
| NGC2437 | 962 | 0.538 |  |
 |
| NGC2516 | 894 | 0.373 |  |
 |
| NGC2682 | 724 | 0.371 |  |
 |
| Pleiades | 721 | 0.478 |  |
 |
| NGC2168 | 709 | 0.629 |  |
 |
| NGC6475 | 612 | 0.373 |  |
 |
| Praesepe | 485 | 0.464 |  |
 |
| IC4651 | 474 | 0.506 |  |
 |
| NGC0188 | 450 | 0.585 |  |
 |
| NGC2360 | 421 | 0.444 |  |
 |
| Stock2 | 410 | 0.802 |  |
 |
| NGC2447 | 377 | 0.267 |  |
 |
| Hyades | 369 | 0.424 |  |
 |
| NGC2422 | 343 | 0.358 |  |
 |
| NGC6281 | 309 | 0.546 |  |
 |
| NGC0884 | 300 | 1.445 |  |
 |
| IC4756 | 299 | 0.597 |  |
 |
| NGC1039 | 296 | 0.400 |  |
 |
| alphaPer | 284 | 0.736 |  |
 |
| NGC2548 | 284 | 0.331 |  |
 |
| NGC6405 | 275 | 0.688 |  |
 |
| NGC0869 | 264 | 1.423 |  |
 |
| IC4725 | 258 | 1.088 |  |
 |
| NGC2423 | 255 | 0.474 |  |
 |
| NGC6025 | 243 | 0.558 |  |
 |
| Blanco1 | 191 | 0.265 |  |
 |
| NGC6633 | 190 | 0.562 |  |
 |
| Trumpler10 | 175 | 0.428 |  |
 |
| NGC7092 | 174 | 0.338 |  |
 |
| IC2602 | 173 | 0.805 |  |
 |
| NGC2451 | 145 | 0.747 |  |
 |
| NGC2323 | 143 | 0.637 |  |
 |
| NGC0752 | 141 | 0.408 |  |
 |
| IC2391 | 134 | 0.732 |  |
 |
| Trumpler02 | 134 | 0.848 |  |
 |
| NGC2158 | 132 | 1.107 |  |
 |
| NGC6774 | 127 | 0.495 |  |
 |
| NGC2547 | 122 | 0.729 |  |
 |
| ComaBer | 109 | 0.257 |  |
 |
| NGC6793 | 103 | 0.962 |  |
 |
| NGC1901 | 71 | 0.407 |  |
 |
| NGC2232 | 70 | 0.681 |  |
 |
| Coll140 | 63 | 0.647 |  |
 |
| NGC3228 | 60 | 0.469 |  |
 |
| IC4665 | 56 | 0.691 |  |
 |
Notes. Clusters are sorted with descending number of member stars. Nearby clusters within 250 pc are marked in bold face. Cluster memberships are taken from Gaia Collaboration (2018a).
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