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Table 1.

Open clusters and OB associations studied in this paper and whose LFs are plotted in Figs. 3 and 4.

Name Ntot Nphot ϖ σϖ Age [Myr] σAge AV σAV
γ-Vel G 134 121 2.9 0.1 9.5 0.5 0.3 0.1
US 1137 994 6.9 0.5 11.5 1.0 0.4 0.1
LS 487 427 5.8 0.2 14.0 1.1 0.2 0.1
UCL-2 202 185 7.0 0.3 17.5 0.5 0.2 0.1
UCL-3 157 147 6.8 0.3 17.5 2.0 0.1 0.1
LCC 1048 989 8.6 0.9 17.5 0.5 0.2 0.1
Col 135 Halo 243 191 3.4 0.3 35.0 1.0 0.3 0.1
UBC 7 206 175 3.6 0.1 35.5 1.1 0.3 0.1
IC 2602 395 326 6.6 0.3 36.5 0.5 0.2 0.1
Platais 8 185 164 7.4 0.3 37.0 1.8 0.3 0.1
IC 2391 296 246 6.6 0.5 37.0 1.7 0.2 0.1
Col 135 200 164 3.3 0.1 40.0 0.8 0.3 0.1
Platais 9 111 109 5.5 0.5 47.0 1.2 0.1 0.1
NGC 2451A 334 285 5.1 0.2 47.0 3.3 0.2 0.1

NGC 6231 268 267 0.61 0.04 4.7 0.4 1.7 0.1

Notes. The meaning of the columns are, from left to right: cluster name, total number of members, number of members used in age determination, median parallax of the cluster in mas, standard deviation of the parallax in mas, the median isochronal age of the cluster in Myr, the uncertainty of the age in Myr, the estimated extinction AV in mag, and the uncertainty of AV in mag.

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