Table B.1
Sample of the information in an online table with information of the clusters analysed in this work.
| Cluster | RA | DEC | E(GBP – GRP) | AG | AV | E(H – K) | E(J – K) | E(GBP – K) | GoodExcess | OC |
|---|---|---|---|---|---|---|---|---|---|---|
| 1636-283 | 249.856 | −28.399 | 2.473 | 5.820 | 4.722 | 0.380 | 0.626 | 5.416 | false | false |
| ADS_16795 | 352.592 | 58.553 | 0.081 | 0.183 | 0.168 | 0.008 | 0.013 | 0.147 | false | true |
| AH03_J0748+26.9 | 117.156 | −26.973 | 0.554 | 1.260 | 1.128 | 0.079 | 0.130 | 1.204 | true | true |
| . | ||||||||||
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| . |
Notes. The table contains some information directly extracted from Hunt & Reffert (2023) (right ascension, RA, declination, DEC and interstellar absorption in V band,
) and others derived in this paper (the median colour of the cluster, 〈GBP – GRP〉, the interstellar absorption in G (using Eq. 2) and V (using Eq. 1) bands,
, using Eq. 2 and 〈GBP – GRP〉 in this table, the colour excesses of the clusters derived using Eqs. 3–5, and two flags indicating if we considered the cluster as an OC and if the colour excess derived can be considered of good quality, according to the filters mentioned in Sect. 5).
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