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Table 4.
Mean post-FDU [C/N] of the open clusters in the GES and APOGEE samples.
| Open clusters | [C/N] | # member stars |
 |
|---|---|---|---|
| (dex) | |||
| GES | |||
| Berkeley 31 | −0.32 ± 0.12 | 1 | 0.87 |
| Berkeley 36 | −0.30 ± 0.26 | 1 | 0.89 |
| Berkeley 44 | −0.38 ± 0.12 | 2 | 1.00 |
| Berkeley 81 | −0.64 ± 0.04 (0.07) | 11 | 0.99 |
| Melotte 71 | −0.65 ± 0.09 | 2 | |
| NGC 2243 | −0.51 ± 0.05 (0.08) | 7 | 1.00 |
| NGC 6005 | −0.64 ± 0.04 (0.05) | 9 | 0.97 |
| NGC 4815 (a) | −0.70 ± 0.11 (0.11) | 5 | |
| NGC 6067 | −0.87 ± 0.04 (0.08) | 9 | 0.99 |
| NGC 6259 | −0.84 ± 0.04 (0.04) | 12 | 0.99 |
| NGC 6802 | −0.67 ± 0.04 (0.08) | 7 | 1.00 |
| Rup 134 | −0.63 ± 0.05 (0.06) | 16 | 0.98 |
| Pismis 18 | −0.74 ± 0.05 (0.03) | 5 | 0.99 |
| Trumpler 23 | −0.68 ± 0.04 (0.04) | 9 | 1.00 |
| Trumpler 20 (a) | −0.60 ± 0.12 (0.12) | 42 | |
| APOGEE | |||
| Berkeley 17 | −0.24 ± 0.02 (0.06) | 7 | |
| Berkeley 53 | −0.52 ± 0.03 (0.05) | 4 | |
| Berkeley 66 | −0.36 ± 0.03 (0.08) | 4 | |
| Berkeley 71 | −0.66 ± 0.04 (0.18) | 7 | |
| FSR0494 | −0.60 ± 0.04 (0.09) | 5 | |
| IC166 | −0.69 ± 0.02 (0.20) | 15 | |
| King 5 | −0.57 ± 0.03 (0.01) | 5 | |
| King 7 | −0.53 ± 0.03 (0.04) | 3 | |
| NGC 1193 | −0.44 ± 0.04 (0.09) | 3 | |
| NGC 1245 | −0.64 ± 0.02 (0.11) | 23 | |
| NGC 1798 | −0.44 ± 0.02 (0.06) | 8 | |
| NGC 188 | −0.32 ± 0.01 (0.04) | 10 | |
| NGC 2158 | −0.41 ± 0.02 (0.13) | 18 | |
| NGC 2420 | −0.40 ± 0.02 (0.07) | 11 | |
| NGC 6791 | −0.20 ± 0.01 (0.06) | 19 | |
| NGC 6811 | −0.68 ± 0.03 (0.01) | 4 | |
| NGC 6819 | −0.49 ± 0.01 (0.03) | 14 | |
| NGC 6866 | −0.69 ± 0.03 (0.06) | 6 | |
| Teutsch 51 | −0.58 ± 0.06 (0.04) | 4 | |
| Trumpler 5 | −0.37 ± 0.02 (0.04) | 9 | |
| NGC 7789 | −0.52 ± 0.01 (0.03) | 17 | |
| GES and APOGEE | |||
| M 67-GES | −0.37 ± 0.07 (0.06) | 3 | |
| M 67-APOGEE DR14 | −0.57 ± 0.01 (0.07) | 23 | |
| M 67-APOGEE DR14 (b) | −0.50 ± 0.09 | 21 | |
| M 67-adopted (DR14 (b)-GES) | −0.43 ± 0.11 | − | |
| NGC 6705-GES (a) | −0.69 ± 0.09 | 27 | |
| NGC 6705-APOGEE DR14 | −0.60 ± 0.01 (0.03) | 12 | |
| NGC 6705-adopted | −0.64 ± 0.09 | − | |
Notes. The values were derived here, with the exception of (a) which is taken from Tautvaišienė et al. (2015), and (b) which we adopted from Souto et al. (2019). 
is the membership probability.
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