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Table 1.

Parameters of the open clusters in the GES sample.

Open clusters RA (a) Dec (a) RGC z RV (b) [Fe/H] (a) log(Age[yr]) Ref. age and distance
(J2000) (kpc) (pc) (km s−1) (dex)
Berkeley 31 06:57:36 +08:16:00 15.16 ± 0.40 +340 ± 30 +56.99 ± 0.14 −0.27 ± 0.06 Cignoni et al. (2011)
Berkeley 36 07:16:06 −13:06:00 11.30 ± 0.20 −40 ± 10 +62.70 ± 0.13 −0.16 ± 0.10 Cignoni et al. (2011)
Berkeley 44 19:17:12 +19:33:00 6.91 ± 0.12 +130 ± 20 −8.71 ± 0.19 +0.27 ± 0.06 Jacobson et al. (2016)
Berkeley 81 19:01:36 −00:31:00 5.49 ± 0.10 −126 ± 7 +48.14 ± 0.26 +0.22 ± 0.07 Magrini et al. (2015)
M 67 08:51:18 +11:48:00 9.05 ± 0.20 +405 ± 40 +34.7 ± 0.9 (a) −0.01 ± 0.04 Salaris et al. (2004)
Melotte 71 07:37:30 −12:04:00 10.50 ± 0.10 +210 ± 20 +50.8 ± 1.3 (a) −0.09 ± 0.03 Salaris et al. (2004)
NGC 2243 06:29:34 −31:17:00 10.40 ± 0.20 +1200 ± 100 +59.65 ± 0.05 −0.38 ± 0.04 Bragaglia & Tosi (2006)
NGC 6005 15:55:48 −57:26:12 5.97 ± 0.34 −140 ± 30 −24.75 ± 0.35 +0.19 ± 0.02 Piatti et al. (1998)
NGC 6067 16:13:11 −54:13:06 6.81 ± 0.12 −55 ± 17 −38.65 ± 0.28 +0.20 ± 0.08 Alonso-Santiago et al. (2017)
NGC 6259 17:00:45 −44:39:18 7.03 ± 0.01 −27 ± 13 −32.98 ± 0.49 +0.21 ± 0.04 Mermilliod et al. (2001)
NGC 6705 18:51:05 −06:16:12 6.33 ± 0.16 −95 ± 10 +35.67 ± 0.19 +0.16 ± 0.04 Cantat-Gaudin et al. (2014)
NGC 6802 19:30:35 +20:15:42 6.96 ± 0.07 +36 ± 3 +13.44 ± 0.60 +0.10 ± 0.02 Jacobson et al. (2016)
Rup 134 17:52:43 −29:33:00 4.60 ± 0.10 −100 ± 10 −40.78 ± 0.15 +0.26 ± 0.06 Carraro et al. (2006)
Pismis 18 13:36:55 −62:05:36 6.85 ± 0.17 +12 ± 2 −27.94 ± 0.29 +0.22 ± 0.04 Piatti et al. (1998)
Trumpler 23 16:00:50 −53:31:23 6.25 ± 0.15 −18 ± 2 −60.74 ± 0.38 +0.21 ± 0.04 Jacobson et al. (2016)
NGC 4815 12:57:59 −64:57:36 6.94 ± 0.04 −95 ± 6 −29.53 ± 0.21 +0.11 ± 0.01 Friel et al. (2014)
Trumpler 20 12:39:32 −60:37:36 6.86 ± 0.01 +134 ± 4 −39.82 ± 0.14 +0.15 ± 0.07 Donati et al. (2014)

Notes.

(b)

RVs are determined with the GIRAFFE sample of high-probability cluster members.

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