Full Table 2 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/468/151

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

ftp://cdsarc.u-strasbg.fr/pub/cats/I/280A

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... $P_{\rm ap}$

$P_{\rm ap}$ is a newly defined combined-membership probability computed for each star in a cluster area by taking only the kinematic and photometric criteria into account, without spatial selection criteria, $P_{\rm ap}={\min}\{P_\mu,P_{\rm ph}\}$ . Note that this definition of the combined-membership probability differs from that of $P_{\rm c}$ used in Paper I.

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.

... CDS

ftp://cdsarc.u-strasbg.fr/pub/cats/J/A+A/438/1163/atlas and ftp://cdsarc.u-strasbg.fr/pub/cats/J/A+A/440/403/atlas

.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.