Table 5
Individual ages, distances, and metallicities for the current sample of open clusters.
| ID | Age | R G | [Fe/H]lit | [Fe/H]rsc | Ref. met. | Ref. age-dist. |
| (Gyrs) | (kpc) | |||||
|
|
||||||
| Be 17 | 10.06 | 10.3 | –0.15 | –0.13 | Friel et al. (2005) | SFa |
| Be 18 | 5.69 | 11.5 | –0.44 | –0.44 | Yong et al. (2012) | SF |
| Be 20 | 4.05 | 15.4 | –0.30 | –0.31 | Sestito et al. (2008) | SF |
| Be 21 | 2.18 | 13.7 | –0.31 | –0.31 | Yong et al. (2012) | SF |
| Be 22 | 4.26 | 11.4 | –0.45 | –0.45 | Yong et al. (2012) | SF |
| Be 25 | 4.00 | 17.6 | –0.20 | –0.22 | Carraro et al. (2007b) | Cb |
| Be 29 | 4.34 | 18.1 | –0.31 | –0.32 | Sestito et al. (2008) | SF |
| Be 31 | 5.32 | 11.5 | –0.53 | –0.49 | Friel et al. (2005) | SF |
| Be 32 | 5.91 | 10.7 | –0.38 | –0.38 | Yong et al. (2012) | SF |
| Be 39 | 7.00 | 11.1 | 0.03 | 0.05 | Friel et al. (2010) | SF |
| Be 66 | 3.98 | 12.0 | –0.48 | –0.46 | Villanova et al. (2005) | SF |
| Be 73 | 1.50 | 16.7 | –0.22 | –0.24 | Carraro et al. (2007b) | C |
| Be 75 | 3.00 | 15.6 | –0.22 | –0.24 | Carraro et al. (2007b) | C |
| Blanco1 | 0.1 | 7.9 | 0.4 | –0.02 | Ford et al. (2005) | W |
| Cr 110 | 1.70 | 9.7 | 0.03 | 0.03 | Pancino et al. (2010) | Bc |
| Cr 261 | 6.00 | 6.9 | 0.13 | 0.12 | Sestito et al. (2008) | B |
| Hyades | 0.70 | 8.0 | 0.11 | 0.11 | Carrera et al. (2011) | SF |
| IC 166 | 2.00 | 10.2 | –0.32 | –0.32 | Friel & Janes (1993) | FJ |
| IC 4651 | 1.68 | 7.1 | 0.11 | 0.15 | Carretta et al. (2004) | SF |
| King 8 | 0.80 | 11.3 | –0.40 | –0.40 | Friel & Janes (1993) | FJ |
| M 67 | 4.30 | 8.5 | –0.01 | 0.01 | Jacobson et al. (2011b) | SF |
| Mel 66 | 5.33 | 8.9 | –0.33 | –0.34 | Sestito et al. (2008) | SF |
| Mel 71 | 0.2 | 10.3 | –0.32 | –0.10 | Brown et al. (1996) | W |
| NGC 1193 | 4.23 | 11.4 | –0.22 | –0.20 | Friel et al. (2010) | SF |
| NGC 1245 | 1.06 | 10.5 | –0.04 | –0.02 | Jacobson et al. (2011b) | SF |
| NGC 1817 | 1.12 | 9.7 | –0.16 | –0.14 | Jacobson et al. (2011b) | SF |
| NGC 188 | 6.30 | 8.8 | –0.03 | –0.01 | Jacobson et al. (2011b) | SF |
| NGC 1883 | 0.65 | 11.7 | –0.01 | 0.01 | Jacobson et al. (2009) | C |
| NGC 1901 | 0.8 | 7.9 | –0.08 | –0.08 | Carraro et al. (2007b) | W |
| NGC 2099 | 0.43 | 9.2 | 0.01 | 0.01 | Pancino et al. (2010) | B |
| NGC 2112 | 2.50 | 8.6 | –0.52 | –0.52 | Friel & Janes (1993) | FJ |
| NGC 2141 | 2.45 | 12.0 | 0.00 | 0.02 | Jacobson et al. (2009) | SF |
| NGC 2158 | 2.00 | 11.5 | –0.28 | –0.26 | Jacobson et al. (2011b) | C |
| NGC 2194 | 0.87 | 10.5 | –0.08 | –0.06 | Jacobson et al. (2011b) | SF |
| NGC 2204 | 2.00 | 11.2 | –0.23 | –0.21 | Jacobson et al. (2011a) | SF |
| NGC 2243 | 4.80 | 10.1 | –0.42 | –0.40 | Jacobson et al. (2011a) | B |
| NGC 2324 | 0.67 | 10.7 | –0.17 | –0.18 | Bragaglia et al. (2008) | SF |
| NGC 2355 | 0.79 | 10.0 | –0.08 | –0.06 | Jacobson et al. (2011b) | SF |
| NGC 2360 | 1.90 | 8.8 | –0.28 | –0.28 | Friel & Janes (1993) | FJ |
| NGC 2420 | 2.20 | 10.0 | –0.20 | –0.18 | Jacobson et al. (2011b) | SF |
| NGC 2425 | 3.55 | 9.5 | –0.15 | –0.13 | Jacobson et al. (2011b) | C |
| NGC 2477 | 1.00 | 8.3 | 0.07 | 0.06 | Bragaglia et al. (2008) | SF |
| NGC 2506 | 1.70 | 10.3 | –0.20 | –0.16 | Carretta et al. (2004) | B |
| NGC 2539 | 0.4 | 8.8 | 0.13 | 0.13 | Santos et al. (2009) | W |
| NGC 2660 | 0.73 | 8.5 | 0.04 | 0.03 | Bragaglia et al. (2008) | SF |
| NGC 2682 | 5.00 | 8.5 | –0.09 | –0.09 | Friel & Janes (1993) | FJ |
| NGC 3680 | 4.00 | 7.8 | –0.16 | –0.16 | Friel & Janes (1993) | FJ |
| NGC 3960 | 0.90 | 7.3 | –0.12 | –0.08 | Bragaglia et al. (2006) | B |
| NGC 5822 | 1.20 | 7.4 | –0.21 | –0.21 | Friel & Janes (1993) | FJ |
| NGC 6134 | 0.93 | 7.1 | 0.15 | 0.19 | Carretta et al. (2004) | Wd |
| NGC 6192 | 0.13 | 6.5 | 0.12 | 0.10 | Magrini et al. (2010) | W |
| NGC 6253 | 3.00 | 6.5 | 0.36 | 0.35 | Sestito et al. (2008) | B |
| NGC 6404 | 0.50 | 6.1 | 0.11 | 0.09 | Magrini et al. (2010) | C |
| NGC 6475 | 0.20 | 7.6 | 0.03 | 0.03 | Villanova et al. (2009) | C |
| NGC 6583 | 1.00 | 5.9 | 0.37 | 0.35 | Magrini et al. (2010) | C |
| NGC 6791 | 8.00 | 7.6 | 0.42 | 0.42 | Geisler et al. (2012) | C |
| NGC 6819 | 2.00 | 7.6 | 0.09 | 0.11 | Bragaglia et al. (2001) | B |
| NGC 6939 | 2.2 | 8.1 | 0.00 | 0.00 | Jacobson et al. (2007) | W |
| NGC 7142 | 4.04 | 9.2 | 0.13 | 0.15 | Jacobson et al. (2008) | SF |
| NGC 752 | 1.24 | 8.2 | 0.08 | 0.08 | Carrera et al. (2011) | SF |
| NGC 7789 | 1.80 | 8.9 | 0.02 | 0.04 | Jacobson et al. (2011b) | SF |
| Praesepe | 0.70 | 8.1 | 0.16 | 0.16 | Carrera et al. (2011) | SF |
| PWM4 | 7.00 | 18.4 | –0.34 | –0.34 | Yong et al. (2012) | YONe |
| Ruprecht 4 | 0.80 | 12.0 | –0.09 | –0.11 | Carraro et al. (2007b) | C |
| Ruprecht 7 | 0.80 | 13.3 | –0.26 | –0.28 | Carraro et al. (2007b) | C |
| Saurer 1 | 5.00 | 20.1 | –0.38 | –0.38 | Carraro et al. (2004) | C |
| To 2 | 2.50 | 14.9 | –0.60 | –0.60 | Friel & Janes (1993) | FJ |
Notes. From left to right the columns give the cluster ID, the Galactocentric distance, the iron abundance available in the literature, the metallicity rescaled to current solar abundance, the references for the metallicity and the references for ages and distances. The acronyms given in Col. 7 refers to SF: (Salaris et al. 2004; Friel 1995), C (Carraro group): (Carraro et al. 2002, 2005a,b,c; Moitinho et al. 2006; Villanova et al. 2007, 2009), B (BOCCE): (Gratton & Contarini 1994; Bragaglia et al. 2001; Kalirai & Tosi 2004; Bragaglia et al. 2006; Carretta et al. 2004, 2005, 2007), W: (WEBDA), and YON: (Yong et al. 2012).
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