Table B.2
Effective temperatures, surface gravities, and global metallicities obtained from the spectroscopic analysis of the observed stars. The CDS version includes all the individual abundances.
| cluster | star | Teff [K] | log ɡ | [M/H] | [Fe/H] |
|---|---|---|---|---|---|
| ASCC23 | 968512002808979456 | 5022 ± 18 | 2.24 ± 0.05 | −0.05 | −0.02 ± 0.06 |
| Alessi 44 | 4240034050119188352 | 4667 ± 10 | 1.69 ± 0.05 | −0.08 | 0.04 ± 0.05 |
| Alessi 62 | 4519333643079413760 | 5027 ± 13 | 2.76 ± 0.03 | −0.02 | 0.07 ± 0.05 |
| Alessi 62 | 4519335601584434048 | 5032 ± 14 | 2.65 ± 0.03 | 0.03 | 0.13 ± 0.05 |
| COIN-Gaia 2 | 423486184872160128 | 5133 ± 16 | 2.72 ± 0.03 | 0.00 | 0.05 ± 0.05 |
| COIN-Gaia 2 | 423487726755535232 | 5144 ± 21 | 2.71 ± 0.06 | −0.03 | 0.02 ± 0.05 |
| COIN-Gaia 6 | 506223988186933888 | 3929 ± 12 | 0.27 ± 0.05 | −0.50 | |
| COIN-Gaia 6 | 506214401820077056 | 5702 ± 30 | 2.61 ± 0.07 | 0.76 | |
| COIN-Gaia 6 | 506224812820610176 | 5489 ± 31 | 2.18 ± 0.07 | 0.58 | |
| FSR0951 | 3344692140944457088 | 5152 ± 13 | 2.63 ± 0.04 | −0.06 | 0.00 ± 0.06 |
| FSR0951 | 3344673277448107776 | 5180 ± 14 | 2.60 ± 0.03 | −0.07 | −0.02 ± 0.05 |
| King 23 | 3109989392447848960 | 4492 ± 15 | 2.07 ± 0.03 | −0.10 | −0.07 ± 0.07 |
| King 23 | 3109989121872110080 | 4619 ± 15 | 2.21 ± 0.03 | −0.07 | −0.02 ± 0.08 |
| NGC 1027 | 465682692367536384 | 4160 ± 14 | 1.07 ± 0.03 | −0.23 | −0.21 ± 0.10 |
| NGC 1647 | 3410117313341005184 | 4696± 11 | 1.81 ± 0.05 | −0.16 | −0.08 ± 0.07 |
| NGC 1647 | 3409869064229856128 | 4914±9 | 1.80 ± 0.02 | −0.13 | −0.04 ± 0.05 |
| NGC 1750 | 3418663507987229184 | 4128±8 | 1.10 ± 0.02 | −0.32 | −0.26 ± 0.06 |
| NGC2186 | 3318650315417696384 | 5686 ± 14 | 1.72 ± 0.04 | −0.05 | 0.04 ± 0.06 |
| NGC 2281 | 951676899239237632 | 4451 ± 8 | 1.74 ± 0.03 | −0.18 | −0.11 ± 0.04 |
| NGC 2281 | 951479674341906560 | 5199 ± 12 | 2.81 ± 0.04 | 0.11 | 0.15 ± 0.08 |
| NGC2345 | 3044665967836430976 | 4251 ± 14 | 1.08 ± 0.04 | −0.26 | −0.23 ± 0.09 |
| NGC2345 | 3044669232011557760 | 4468 ± 13 | 1.28 ± 0.05 | −0.16 | −0.11 ± 0.09 |
| NGC 2358 | 2934861658580860928 | 5044 ± 11 | 2.57 ± 0.02 | −0.09 | −0.02 ± 0.05 |
| NGC 2358 | 2934838637556373888 | 5129 ± 13 | 2.62 ± 0.03 | −0.04 | 0.03 ± 0.05 |
| NGC 2358 | 2934834411308570624 | 5155 ± 11 | 2.88 ± 0.03 | −0.07 | 0.00 ± 0.04 |
| NGC7654 | 2015645057006454144 | 4001 ± 12 | 0.18 ± 0.04 | −0.38 | |
| NGC7654 | 2015663649928489856 | 6072 ± 16 | 1.16 ± 0.03 | −0.19 | −0.05 ± 0.09 |
| Stock 1 | 2024990807120270976 | 4996 ± 17 | 2.58 ± 0.03 | 0.06 | 0.15 ± 0.07 |
| Trumpler2 | 454676374812927744 | 4071 ± 7 | 0.83 ± 0.03 | −0.40 | −0.34 ± 0.05 |
| Trumpler2 | 457691785453711360 | 4370±8 | 1.30 ± 0.03 | −0.26 | −0.19 ± 0.04 |
| UBC54 | 233820772674404736 | 5064 ± 19 | 2.47 ± 0.03 | −0.04 | 0.05 ± 0.05 |
| UBC 54 | 233049705784504576 | 5089 ± 14 | 2.27 ± 0.04 | −0.05 | 0.01 ± 0.05 |
Notes. We also list the iron abundances computed with respect to the Sun ([Fe/H]). The stars without abundance values correspond to the two identified supergiants (COIN-Gaia 6 and NGC 7654), and the two stars with low S/N are from COIN-Gaia 6, as discussed in Sect 4.2.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.