\begin{table}%t8
\caption{\label{vr67M}The cross-identification of stars considered as candidate members by us, 
with the radial velocities sudies by \cite{Mathieu, Mathieu90} and
the comparison of those with the parametric ($P_{\rm P}$) and 
non-parametric ($P_{\rm NP}$) probabilities. 
See text for explanation of the agreement index $P_{\rm c}$. }
 {
%\begin{center}
\par
\begin{tabular}{cccccccccccc}
\hline
ID$_{\rm BDA}$ & ID$_{\rm Zhao}$ & $P_{\rm P}$ & $P_{\rm NP}$ & $P_{\rm c}$ & $Vr^*$ & 
ID$_{\rm BDA}$ & ID$_{\rm Zhao}$ & $P_{\rm P}$ & $P_{\rm NP}$ & $P_{\rm c}$ & $Vr^*$  \\
\hline
4 & 818 & 0.94 & 0.96 & 3 & 34.0 $\pm$2.0 &        185 & 958 & 0.79 & 0.94 & 3 & 33.4 $\pm$0.0  \\
  16 & 829 & 0.88 & 0.96 & 3 & 33.2 $\pm$0.9 &    190 & 989 & 0.80 & 0.94 & 0 & 43.6 $\pm$0.0 SB \\ 
18 & 521 & 0.92 & 0.95 & 3 & 32.9 $\pm$0.5 &       192 & 603 & 0.98 & 0.97 & 3 & 32.7 $\pm$1.1 \\ 
  20 & 834 & 0.96 & 0.97 & 3 & 33.1 $\pm$1.0 &    193 & 999 & 0.98 & 0.97 & 3 & 33.7 $\pm$0.5 \\    
22 & 839 & 0.95 & 0.96 & 3 & 34.4 $\pm$1.9 SB1 &   195 &1017 & 0.97 & 0.98 & 3 & 33.87$\pm$0.12 SB1\\
  28 & 840 & 0.97 & 0.97 & 3 & 33.7 $\pm$1.0 &    210 &1005 & 0.98 & 0.97 & 3 & 33.9 $\pm$1.1 \\    
30 & 845 & 0.97 & 0.97 & 3 & 33.6 $\pm$0.4 &       215 & 608 & 0.98 & 0.98 & 3 & 33.6 $\pm$0.6 \\
  37 & 846 & 0.97 & 0.97 & 3 & 33.7 $\pm$0.3 &    216 &1010 & 0.97 & 0.98 & 3 & 33.03$\pm$0.13 SB1 \\
46 & 843 & 0.98 & 0.97 & 3 & 33.8 $\pm$0.1 &       217 &1002 & 0.97 & 0.97 & 3 & 33.3 $\pm$0.4 \\
  48 & 848 & 0.96 & 0.98 & 3 & 33.0 $\pm$0.4 &    218 &1006 & 0.98 & 0.97 & 3 & 34.0 $\pm$0.5 \\    
51 & 849 & 0.96 & 0.97 & 3 & 34.6 $\pm$0.9 &       219 &1007 & 0.98 & 0.98 & 3 & 33.4 $\pm$0.3 SB1\\
  54 & 863 & 0.95 & 0.97 & 3 & 34.5 $\pm$0.7 &    223 & 609 & 0.68 & 0.94 & 3 & 32.8 $\pm$0.4 \\    
55 & 862 & 0.75 & 0.92 & 0 & 42.1 $\pm$0.0 SB &    224 &1011 & 0.95 & 0.96 & 3 & 32.55$\pm$0.07 SB1\\
  72 & 876 & 0.97 & 0.98 & 3 & 33.3 $\pm$0.6 &    226 &1013 & 0.98 & 0.98 & 3 & 32.5 $\pm$1.0 \\    
79 & 860 & 0.97 & 0.98 & 3 & 34.1 $\pm$1.7 &       227 &1004 & 0.98 & 0.97 & 3 & 32.8 $\pm$0.7 \\
  84 & 966 & 0.78 & 0.94 & 3 & 34.1 $\pm$0.4 &    231 &1029 & 0.97 & 0.97 & 3 & 32.5 $\pm$0.6 \\    
86 & 933 & 0.81 & 0.86 & 1 & 27.6 $\pm$0.0 &       236 &1025 & 0.98 & 0.98 & 3 & 33.82$\pm$0.18 SB1\\
  88 & 927 & 0.96 & 0.97 & 3 & 34.13$\pm$0.23 SB2&237 & 611 & 0.97 & 0.98 & 3 & 34.7 $\pm$0.7 \\    
95 & 886 & 0.98 & 0.98 & 3 & 34.7 $\pm$2.4 &       238 &1028 & 0.75 & 0.94 & 3 & 38.3 $\pm$0.0 \\
  96 & 929 & 0.96 & 0.98 & 3 & 33.1 $\pm$0.7 &    241 &1027 & 0.96 & 0.96 & 3 & 33.2 $\pm$0.7 \\    
101 & 930 & 0.97 & 0.98 & 3 & 32.9 $\pm$0.9  &     243 &1026 & 0.96 & 0.96 & 3 & 33.4 $\pm$0.5 \\
 102 & 893 & 0.98 & 0.97 & 3 & 36.17$\pm$0.17 SB1&244 &1032 & 0.93 & 0.96 & 3 & 33.55$\pm$0.05 SB1 \\
104 & 931 & 0.95 & 0.97 & 3 & 33.5 $\pm$0.4  &     248 & 612 & 0.98 & 0.98 & 3 & 34.0 $\pm$1.3 \\
 105 & 883 & 0.80 & 0.94 & 3 & 34.3 $\pm$0.7 &    252 & 618 & 0.97 & 0.96 & 3 & 32.5 $\pm$1.0 \\    
108 & 894 & 0.51 & 0.93 & 2 & 34.7 $\pm$0.6  &     255 &1043 & 0.96 & 0.97 & 3 & 31.3 $\pm$0.3 \\
 111 & 891 & 0.98 & 0.97 & 3 & 33.70$\pm$0.22 SB1&256 & 226 & 0.96 & 0.98 & 3 & 33.2 $\pm$0.9 \\    
115 & 918 & 0.97 & 0.98 & 3 & 34.4 $\pm$0.5  &     262 &1046 & 0.97 & 0.97 & 3 & 31.6 $\pm$0.7 \\
 117 & 887 & 0.98 & 0.98 & 3 & 34.4 $\pm$0.3 SB2 &266 & 647 & 0.78 & 0.94 & 3 & 34.3 $\pm$0.4 \\    
119 & 924 & 0.97 & 0.97 & 3 & 34.34$\pm$0.21 SB2 & 271 &1058 & 0.93 & 0.96 & 3 & 34.1 $\pm$0.8 \\
 124 & 912 & 0.97 & 0.98 & 3 & 29.6 $\pm$0.7 SB & 272 & 645 & 0.97 & 0.97 & 3 & 31.8 $\pm$0.4 \\    
127 & 911 & 0.97 & 0.98 & 3 & 33.3 $\pm$0.8  &     281 &1060 & 0.96 & 0.97 & 3 & 33.4 $\pm$0.8 \\
 130 & 910 & 0.94 & 0.98 & 3 & 33.7 $\pm$0.7 &    286 & 697 & 0.35 & 0.92 & 2 & 33.6 $\pm$0.5 \\    
131 & 972 & 0.95 & 0.96 & 3 & 33.3 $\pm$2.0 SB2 &  287 & 698 & 0.98 & 0.97 & 3 & 32.8 $\pm$0.5 \\
 134 & 907 & 0.98 & 0.97 & 3 & 32.5 $\pm$1.2 SB1& 289 & 683 & 0.94 & 0.96 & 3 & 32.7 $\pm$0.4 \\    
135 & 908 & 0.97 & 0.97 & 3 & 34.3 $\pm$0.6  &     291 & 700 & 0.96 & 0.97 & 3 & 34.1 $\pm$0.1 \\
 136 & 974 & 0.94 & 0.96 & 3 & 32.87$\pm$0.12 SB1&305 & 133 & 0.52 & 0.92 & 2 & 34.2 $\pm$0.9 \\    
141 & 947 & 0.86 & 0.95 & 3 & 33.6 $\pm$0.4  &     1182 & 174 & 0.95 & 0.98 & 3 & 34.6 $\pm$0.9 \\
 143 & 937 & 0.91 & 0.96 & 3 & 32.93$\pm$0.07 SB1&2079& 172 & 0.98 & 0.98 & 3 & 34.4 $\pm$0.5 \\    
149 & 949 & 0.98 & 0.97 & 3 & 35.5 $\pm$0.8  &     2087 & 211 & 0.94 & 0.97 & 3 & 31.5 $\pm$3.0\\
 151 & 971 & 0.81 & 0.94 & 3 & 33.9 $\pm$0.5 &    3035 &1001 & 0.98 & 0.98 & 3 & 34.1 $\pm$0.5 \\   
157 & 976 & 0.98 & 0.98 & 3 & 33.6 $\pm$0.5  &     3116 & 642 & 0.98 & 0.97 & 3 & 33.60$\pm$0.13 SB1\\
 163 & 995 & 0.98 & 0.98 & 3 & 33.8 $\pm$0.8 &    4004 & 939 & 0.98 & 0.98 & 3 & 33.48$\pm$0.19 SB2\\
164 & 983 & 0.79 & 0.94 & 3 & 33.3 $\pm$0.4  &     4096 & 578 & 0.97 & 0.97 & 3 & 34.0 $\pm$0.8 \\
 166 &   4 & 0.97 & 0.98 & 3 & 33.3 $\pm$0.3 &    7591 & 135 & 0.91 & 0.96 & 3 & 33.4 $\pm$0.8  \\ 
170 & 953 & 0.60 & 0.93 & 3 & 33.59$\pm$0.10 SB1 & 7657 & 505 & 0.28 & 0.87 & 2 & 33.2 $\pm$0.9 \\
 174 & 961 & 0.97 & 0.98 & 3 & 36.2 $\pm$4.5&     8402 & 231 & 0.83 & 0.94 & 3 & 33.6 $\pm$0.4 \\   
176 & 914 & 0.97 & 0.98 & 3 & 32.5 $\pm$0.4 SB1 &  8524 & 639 & 0.69 & 0.89 & 3 & 33.6 $\pm$0.7 \\
 180 & 985 & 0.98 & 0.97 & 3 & 35.0 $\pm$0.8 &    8571 & 253 & 0.94 & 0.95 & 3 & 34.2 $\pm$0.4 \\   
181 & 955 & 0.98 & 0.98 & 3 & 33.3 $\pm$0.7 &      8792 & 282 & 0.85 & 0.93 & 3 & 33.1 $\pm$0.5 \\
 182 & 956 & 0.97 & 0.98 & 3 & 32.2 $\pm$2.2 &    8808 & 277 & 0.85 & 0.94 & 3 & 29.6 $\pm$1.0 \\   
184 & 987 & 0.98 & 0.97 & 0 & 61.4 $\pm$0.0&       8832 & 713 & 0.97 & 0.97 & 3 & 33.5 $\pm$0.7 \\
\hline
\end{tabular}
%\end{center}
\par
(*) Zero errors mean that only one measurement was taken and no dispersion 
could be calculated. SB1: Single-lined spectroscopic binary. 
SB2: Double-lined spectroscopic binary.
}
\end{table}