Open Access
Table D.1
Differences of the atmospheric parameters and abundances for the OCs in common with the literature.
| OC | Teff (K) | log ɡ (dex) | N | [Fe/H] | [Mg/Fe] | [Si/Fe] | [Ti/Fe] | [Na/Fe] | [Al/Fe] | [Mn/Fe] | [Co/Fe] | [Ni/Fe] | [Sr/Fe] | [Y/Fe] | [Eu/Fe] | Reference |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| New in SPA | ||||||||||||||||
| IC 4756 | 8 ± 84 | 0.58 ± 0.24 | 2 | 0.15 | - | -0.36 | - | -0.48 | -0.34 | - | - | -0.03 | - | - | - | Jacobson et al. (2007) |
| -69 ± 5 | 0.00 ± 0.01 | 2 | -0.03 | - | - | - | - | - | - | - | - | - | - | - | Santos et al. (2009) | |
| - | - | - | -0.04 | 0.02 | -0.08 | 0.15 | 0.10 | - | - | -0.11 | 0.06 | - | - | - | Smiljanic et al. (2009) | |
| -65 ± 12 | 0.01 ± 0.08 | 2 | -0.08 | - | -0.12 | 0.00 | -0.10 | -0.02 | - | - | 0.01 | - | - | - | Pace et al. (2010) | |
| -138 ± 90 | -0.49 ± 0.34 | 6 | 0.01 | -0.15 | -0.15 | - | -0.12 | -0.17 | - | - | 0.02 | - | - | - | Ting et al. (2012) | |
| -48 ± 46 | 0.27 ± 0.11 | 8 | 0.02 | -0.11 | -0.06 | 0.10 | -0.05 | -0.09 | 0.10 | -0.01 | 0.11 | - | 0.22 | 0.05 | Bagdonas et al. (2018) | |
| -71 ± 87 | -0.09 ± 0.20 | 4 | -0.00 | 0.01 | -0.02 | 0.07 | - | - | - | - | 0.08 | - | - | - | Casamiquela et al. (2017, 2019) | |
| - | - | - | 0.05 | -0.05 | -0.08 | - | - | 0.10 | - | - | - | - | - | - | Ray et al. (2022) | |
| 50 ± 49 | 0.21 ± 0.11 | 8 | - | - | - | - | - | - | 0.10 | - | - | - | - | - | Tsantaki et al. (2023) | |
| -43 ± 35 | 0.05 ± 0.09 | 4 | 0.03 | 0.02 | -0.07 | 0.11 | -0.06 | -0.09 | 0.17 | -0.01 | 0.09 | -0.15 | 0.20 | - | Carbajo-Hijarrubia et al. (2024) | |
| NGC 6991 | - | - | - | 0.03 | 0.01 | -0.04 | 0.15 | -0.07 | -0.14 | 0.08 | -0.06 | 0.07 | - | 0.15 | -0.07 | Reddy & Lambert (2019) |
| 10 | 0.27 | 1 | 0.03 | -0.04 | -0.02 | 0.07 | - | - | - | - | 0.09 | - | - | - | Casamiquela et al. (2017, 2019) | |
| - | - | - | 0.07 | -0.02 | -0.06 | 0.10 | -0.11 | -0.12 | 0.15 | -0.03 | 0.06 | -0.16 | 0.16 | - | Carbajo-Hijarrubia et al. (2024) | |
| NGC 752 | - | - | - | 0.01 | - | - | - | - | - | - | - | - | - | - | - | Sestito et al. (2004) |
| 87 | -0.29 | 1 | -0.06 | -0.17 | -0.01 | 0.14 | -0.01 | 0.05 | - | -0.05 | 0.06 | - | 0.24 | - | Carrera & Pancino (2011) | |
| 59 ± 31 | 0.36 ± 0.08 | 2 | 0.06 | -0.04 | -0.10 | 0.16 | -0.12 | -0.22 | 0.18 | -0.02 | 0.06 | - | 0.18 | 0.01 | Reddy et al. (2012) | |
| 67 ± 47 | 0.36 ± 0.12 | 3 | 0.01 | 0.04 | -0.10 | 0.15 | -0.05 | -0.10 | 0.28 | 0.08 | 0.03 | - | 0.27 | 0.03 | Böcek Topcu et al. (2015) | |
| 29 ± 10 | 0.13 ± 0.01 | 2 | 0.01 | -0.03 | -0.01 | 0.07 | - | - | - | - | 0.03 | - | - | - | Casamiquela et al. (2017, 2019) | |
| -91 ± 31 | 0.31 ± 0.06 | 2 | 0.03 | -0.09 | -0.06 | 0.01 | 0.09 | -0.27 | 0.06 | -0.15 | 0.07 | - | 0.19 | - | Lum & Boesgaard (2019) | |
| - | - | - | 0.06 | 0.04 | 0.04 | 0.17 | -0.05 | -0.11 | 0.05 | 0.10 | 0.05 | - | - | - | Spina et al. (2021) | |
| - | - | - | 0.08 | -0.05 | 0.02 | 0.15 | -0.11 | -0.09 | 0.01 | 0.02 | 0.08 | - | - | - | Myers et al. (2022) | |
| - | - | - | 0.06 | 0.04 | 0.03 | 0.17 | -0.04 | -0.02 | 0.03 | 0.07 | 0.08 | - | - | - | Donor et al. (2020) | |
| -8 ± 11 | 0.17 ± 0.05 | 2 | 0.04 | -0.01 | -0.05 | 0.09 | -0.10 | -0.14 | 0.14 | -0.01 | 0.08 | -0.09 | 0.18 | - | Carbajo-Hijarrubia et al. (2024) | |
| UBC 3 | -73 | 0.23 | 1 | 0.01 | -0.11 | -0.18 | 0.02 | -0.15 | -0.09 | 0.04 | -0.10 | -0.00 | -0.26 | 0.11 | - | Carbajo-Hijarrubia et al. (2024) |
| SPA previous studies | ||||||||||||||||
| Collinder 350 | 55 ± 59 | 0.26 ± 0.06 | 2 | 0.00 | -0.13 | -0.08 | -0.05 | -0.16 | 0.03 | - | -0.07 | -0.07 | - | 0.25 | 0.23 | Casali et al. (2020a) |
| 10 ± 174 | 0.22 ± 0.21 | -0.03 | ||||||||||||||
| Gulliver 51 | 156 | -0.31 | 1 | -0.09 | -0.10 | 0.04 | 0.05 | -0.13 | -0.11 | - | -0.06 | 0.00 | - | 0.02 | 0.03 | |
| 66 | -0.52 | -0.014 | ||||||||||||||
| NGC 7044 | -34± 83 | 0.14 ± 0.14 | 4 | - | - | - | - | - | - | - | - | - | - | - | - | |
| 28 ± 73 | -0.25 ± 0.09 | -0.05 | ||||||||||||||
| Ruprecht 171 | -136 ± 131 | -0.22 ± 0.32 | 7 | -0.13 | -0.03 | 0.00 | 0.02 | -0.09 | 0.00 | - | -0.13 | -0.05 | - | 0.13 | 0.10 | |
| -25 ± 113 | -0.24 ± 0.14 | -0.10 | ||||||||||||||
| Alessi 1 | -166 ± 125 | -0.23 ± 0.31 | 4 | -0.01 | 0.11 | -0.14 | 0.15 | 0.12 | 0.11 | - | - | - | - | - | - | Zhang et al. (2021, 2022) |
| Alessi Teutsch 11 | -43 | 0.051 | 1 | 0.15 | 0.07 | -0.25 | 0.15 | -0.12 | 0.02 | - | - | - | - | - | - | |
| Basel 11 b | -211 ± 20 | -0.45 ± 0.18 | 3 | 0.04 | 0.08 | -0.17 | 0.05 | 0.00 | 0.07 | - | - | - | - | - | - | |
| COIN-Gaia30 | -404 | -0.99 | 1 | -0.07 | 0.11 | -0.09 | -0.08 | -0.04 | 0.06 | - | - | - | - | - | - | |
| Collinder 350 | -60 ± 80 | 0.13 ± 0.31 | 2 | 0.16 | -0.10 | -0.10 | -0.05 | -0.07 | 0.01 | - | - | - | - | - | - | |
| Collinder 463 | -134 ± 54 | -0.20 ± 0.13 | 2 | 0.09 | 0.07 | -0.18 | 0.11 | -0.05 | 0.06 | - | - | - | - | - | - | |
| Gulliver 18 | -401 | -0.98 | 1 | 0.09 | 0.22 | -0.21 | -0.16 | -0.05 | -0.14 | - | - | - | - | - | - | |
| Gulliver 24 | -191 | -0.73 | 1 | 0.04 | 0.19 | -0.29 | 0.02 | 0.08 | -0.02 | - | - | - | - | - | - | |
| NGC 2437 | -184 ± 80 | -0.34 ± 0.17 | 5 | -0.03 | 0.10 | -0.16 | 0.07 | 0.06 | -0.00 | - | - | - | - | - | - | |
| NGC 2509 | 68 | 0.35 | 1 | 0.31 | 0.06 | -0.17 | 0.18 | -0.09 | -0.08 | - | - | - | - | - | - | |
| NGC 2548 | -156 ± 149 | -0.22 ± 0.46 | 3 | 0.07 | 0.10 | -0.06 | 0.06 | 0.08 | 0.07 | - | - | - | - | - | - | |
| NGC 2682 | -71 ± 157 | 0.03 ± 0.30 | 2 | 0.05 | 0.05 | -0.06 | 0.19 | 0.04 | 0.05 | - | - | - | - | - | - | |
| NGC 7209 | -168 | 0.37 | 1 | 0.01 | 0.07 | -0.15 | 0.04 | 0.17 | -0.00 | - | - | - | - | - | - | |
| Tombaugh 5 | -197 ± 223 | -0.44 0.56 ± | 3 | 0.00 | 0.08 | -0.16 | -0.05 | -0.11 | 0.10 | - | - | - | - | - | - | |
| UPK 219 | -290 | -0.54 | 1 | 0.05 | 0.05 | -0.20 | -0.09 | -0.23 | 0.00 | - | - | - | - | - | - | |
| Stock 2 | -42 ± 238 | -0.23 ± 0.37 | 8 | 0.05 | 0.10 | -0.13 | 0.06 | -0.05 | 0.09 | 0.04 | -0.12 | -0.01 | -0.06 | 0.01 | - | Alonso-Santiago et al. (2021) |
| Literature | ||||||||||||||||
| Basel 11b | - | - | - | 0.04 | -0.04 | -0.09 | 0.06 | 0.03 | 0.06 | -0.11 | -0.02 | 0.01 | - | - | - | Donor et al. (2020) |
| - | - | - | 0.07 | 0.02 | -0.07 | 0.06 | -0.06 | -0.01 | -0.14 | 0.02 | -0.02 | - | - | - | Spina et al. (2021) | |
| Collinder 350 | 36 | 0.09 | 1 | -0.14 | -0.13 | -0.12 | 0.07 | - | -0.04 | - | -0.03 | 0.02 | - | 0.24 | 0.18 | Pakhomov et al. (2009) |
| - | - | - | 0.07 | -0.16 | -0.15 | -0.07 | - | - | - | -0.08 | -0.07 | - | 0.11 | - | Blanco-Cuaresma et al. (2015) | |
| - | - | - | -0.06 | -0.01 | 0.02 | -0.03 | - | 0.10 | - | 0.01 | -0.03 | - | 0.11 | 0.18 | Blanco-Cuaresma & Fraix-Burnet(2018) | |
| Stock 2 | 36 ± 68 | 0.31 ± 0.13 | 2 | 0.04 | -0.13 | -0.17 | 0.07 | -0.18 | -0.10 | 0.04 | -0.10 | -0.02 | - | 0.22 | 0.01 | Reddy & Lambert (2019) |
| NGC 2548 | 102 | -1.96 | 1 | - | - | - | - | - | - | - | - | - | - | - | - | Sun et al. (2020) |
| -24 | 0.17 | 1 | 0.04 | -0.01 | 0.00 | -0.03 | -0.11 | -0.11 | -0.02 | -0.06 | -0.05 | - | 0.26 | 0.-11 | Spina et al. (2021) | |
| NGC 2632 | - | - | - | 0.03 | 0.07 | 0.07 | 0.08 | 0.20 | -0.05 | 0.06 | 0.08 | 0.12 | - | 0.08 | - | Spina et al. (2021) |
| -144 ± 69 | -0.12 ± 0.17 | 2 | -0.07 | 0.01 | -0.03 | 0.08 | -0.06 | -0.18 | 0.16 | -0.07 | 0.05 | -0.19 | 0.05 | - | Carbajo-Hijarrubia et al. (2024) | |
| NGC 2682 | - | - | - | 0.07 | -0.07 | -0.07 | 0.10 | -0.13 | -0.13 | - | -0.06 | 0.05 | - | - | - | Tautvaišiene et al. (2000) |
| - | - | - | 0.02 | -0.13 | -0.06 | 0.02 | -0.24 | -0.16 | - | - | 0.01 | - | - | - | Yong et al. (2006) | |
| - | - | - | -0.01 | -0.24 | -0.07 | 0.18 | -0.02 | -0.02 | - | -0.06 | 0.04 | - | 0.14 | - | Pancino et al. (2010) | |
| - | - | - | 0.01 | -0.02 | -0.15 | 0.28 | -0.07 | -0.10 | - | 0.18 | 0.11 | - | - | - | Friel et al. (2010) | |
| 22 ± 6 | 0.15 ± 0.09 | 2 | 0.05 | -0.20 | -0.18 | 0.24 | 0.03 | - | - | - | 0.10 | - | - | - | Jacobson et al. (2011) | |
| -87 ± 28 | 0.01 ± 0.08 | 2 | 0.08 | 0.03 | 0.01 | - | 0.03 | -0.00 | - | - | - | - | - | - | Gao et al. (2018) | |
| -32 ± 18 | 0.04 ± 0.02 | 2 | 0.01 | 0.02 | -0.02 | 0.10 | - | - | - | - | 0.03 | - | - | - | Casamiquela et al. (2017, 2019) | |
| - | - | - | 0.04 | 0.03 | 0.02 | 0.14 | 0.01 | -0.03 | 0.02 | -0.28 | 0.10 | - | 0.06 | 0.04 | Spina et al. (2021) | |
| - | - | - | 0.03 | 0.03 | 0.03 | 0.15 | 0.02 | 0.02 | 0.02 | 0.04 | 0.07 | - | - | - | Donor et al. (2020) | |
| -94 ± 14 | 0.01 ± 0.01 | 2 | 0.01 | 0.02 | -0.08 | 0.10 | -0.15 | -0.14 | 0.11 | -0.03 | 0.02 | -0.12 | 0.16 | - | Carbajo-Hijarrubia et al. (2024) | |
| Ruprecht 171 | -220 ± 36 | -0.20 ± 0.08 | 3 | -0.22 | 0.01 | -0.02 | 0.02 | -0.10 | -0.13 | 0.03 | -0.02 | -0.07 | 0.07 | 0.15 | - | Carbajo-Hijarrubia et al. (2024) |
| Tombaugh 5 | 25 | 0.27 | 1 | -0.04 | - | -0.07 | -0.07 | - | - | - | - | -0.10 | - | - | - | Baratella et al. (2018) |
Notes: For the Casali et al. (2020a), the first difference value in Teff, log ɡ and [Fe/H] is related to FAMA and the second to ROTFIT results.
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