\begin{table}%t4%t5
\caption{\label{table:pdfparameters}The results obtained for all the extracted fields in the PM2000~zone.}
%\centering
\par
\begin{tabular}{lrrrrrrrrrr}
\hline\hline \noalign{\smallskip}
Cluster & 
$\mu_{\alpha,c}$ & $\mu_{\delta,c}$ & 
$\mu_{\alpha,f}$  & $\mu_{\delta,f}$ &  
$\sigma_{\mu_{\alpha, f}}$ & $\sigma_{\mu_{\delta, f}}$ &
$\rho_f$ & $n_c$ & $n_{\rm memb}$&Class\\
\hline
\multicolumn{11}{c}{Good} \\ 
NGC 2682 &$   -8.23\pm0.05 $&$   -5.72\pm0.05 $&$  -4.15\pm0.30 $&$   -5.84\pm0.25 $&$   7.20\pm0.22 $&$   6.29\pm0.20 $&$  -0.17\pm0.04 $&$   0.40\pm0.02$      &        502 & A\\
Berkeley 82 &$    3.02\pm0.61 $&$   -1.64\pm0.48 $&$  -0.13\pm0.73 $&$   -2.15\pm1.24 $&$   1.00\pm 0.00 $&$   3.50\pm1.47 $&$   0.31\pm0.22 $&$   0.33\pm0.19$   &         16 & B\\
NGC 1817 &$    2.66\pm0.18 $&$   -3.72\pm0.19 $&$   3.56\pm0.56 $&$   -6.70\pm0.67 $&$   7.16\pm0.49 $&$   8.59\pm0.54 $&$  -0.09\pm0.06 $&$   0.72\pm0.03$      &        836 & B\\
NGC 2169 &$   -2.72\pm0.40 $&$   -4.34\pm0.41 $&$  -3.64\pm3.58 $&$  -11.46\pm4.61 $&$   9.30\pm2.69 $&$  10.75\pm3.14 $&$  -0.44\pm0.29 $&$   0.86\pm0.06$      &         90 & B\\
NGC 2194 &$    0.07\pm0.20 $&$   -2.69\pm0.29 $&$  -0.31\pm0.26 $&$   -3.60\pm0.33 $&$   3.74\pm0.20 $&$   4.79\pm0.25 $&$  -0.08\pm0.06 $&$   0.21\pm0.04$      &         65 & B\\
NGC 2304 &$   -1.78\pm0.66 $&$   -5.77\pm0.68 $&$   0.89\pm1.28 $&$   -2.41\pm1.51 $&$   3.54\pm1.23 $&$   4.91\pm1.31 $&$  -0.52\pm0.19 $&$   0.64\pm0.13$      &         78 & B\\
NGC 2355 &$   -0.39\pm0.32 $&$   -4.78\pm0.30 $&$   1.03\pm0.98 $&$   -7.73\pm0.91 $&$   7.73\pm0.79 $&$   6.75\pm0.71 $&$  -0.22\pm0.10 $&$   0.64\pm0.06$      &        213 & B\\
\hline
\multicolumn{11}{c}{Intermediate} \\ 
Chupina 1 &$  -10.54\pm0.26 $&$   -3.52\pm0.21 $&$  -3.59\pm1.02 $&$   -3.17\pm0.95 $&$   5.76\pm0.71 $&$   5.75\pm0.71 $&$  -0.09\pm0.16 $&$   0.30\pm0.07$     &         22 & B\\
Chupina 2 &$    5.84\pm0.59 $&$  -12.50\pm0.69 $&$  -8.58\pm1.09 $&$   -6.68\pm1.19 $&$   3.61\pm0.73 $&$   3.96\pm1.05 $&$  -0.78\pm0.10 $&$   0.13\pm0.09$     &          3 & B\\
Chupina 3 &$   -7.32\pm0.25 $&$   -4.37\pm0.22 $&$   3.18\pm2.48 $&$   -6.55\pm2.35 $&$   5.06\pm2.05 $&$   5.90\pm1.65 $&$  -0.38\pm0.32 $&$   0.65\pm0.12$     &         17 & B\\
Chupina 4 &$   -9.91\pm0.37 $&$   -5.05\pm0.30 $&$  -2.06\pm1.11 $&$   -5.13\pm1.37 $&$   5.73\pm0.81 $&$   7.86\pm1.04 $&$  -0.27\pm0.15 $&$   0.23\pm0.08$     &         12 & B\\
Chupina 5 &$   -8.68\pm0.35 $&$   -6.90\pm0.31 $&$  -3.12\pm1.19 $&$   -8.28\pm1.11 $&$   5.05\pm0.81 $&$   5.34\pm0.87 $&$   0.07\pm0.19 $&$   0.32\pm0.11$     &         15 & B\\
NGC 7036 &$   -5.04\pm0.41 $&$   -6.84\pm0.35 $&$   0.06\pm1.26 $&$   -8.15\pm1.11 $&$   8.23\pm0.98 $&$   7.33\pm0.93 $&$   0.56\pm0.09 $&$   0.26\pm0.08$      &         20 & B\\
Roslund 1 &$   -0.06\pm0.52 $&$   -5.09\pm0.55 $&$  -1.74\pm1.06 $&$   -7.22\pm1.17 $&$   7.18\pm0.89 $&$   8.12\pm0.99 $&$  -0.08\pm0.12 $&$   0.47\pm0.08$     &         70 & B\\
Berkeley 43 &$    0.30\pm0.78 $&$   -1.81\pm0.68 $&$  -0.36\pm1.02 $&$   -3.52\pm1.65 $&$   4.38\pm1.02 $&$   8.13\pm1.31 $&$   0.08\pm0.16 $&$   0.36\pm0.15$   &         23 & C\\
Berkeley 45 &$   -1.01\pm0.96 $&$   -9.27\pm0.94 $&$   6.28\pm1.13 $&$   -3.94\pm1.39 $&$   2.44\pm1.17 $&$   3.75\pm1.10 $&$  -0.37\pm0.33 $&$   0.47\pm0.12$   &         42 & C\\
Berkeley 47 &$    0.90\pm0.90 $&$   -4.14\pm0.86 $&$   1.97\pm1.93 $&$   -4.93\pm2.46 $&$   6.79\pm1.63 $&$   9.65\pm2.05 $&$   0.65\pm0.14 $&$   0.60\pm0.12$   &         35 & C\\
King 26 &$    3.80\pm0.58 $&$   -5.72\pm0.47 $&$   1.18\pm1.99 $&$   -6.31\pm1.73 $&$   7.68\pm1.72 $&$   6.50\pm1.58 $&$   0.04\pm0.22 $&$   0.45\pm0.15$       &         21 & C\\
Skiff J0614+129 &$   -0.31\pm0.29 $&$   -2.73\pm0.37 $&$  -0.57\pm0.44 $&$   -4.31\pm0.63 $&$   4.48\pm0.32 $&$   6.56\pm0.47 $&$  -0.05\pm0.09 $&$   0.18\pm0.05$ &       29 & C\\
NGC 1807 &$    2.06\pm0.23 $&$   -4.56\pm0.24 $&$   3.57\pm0.68 $&$   -7.83\pm0.75 $&$   7.80\pm0.57 $&$   8.35\pm0.59 $&$  -0.08\pm0.07 $&$   0.66\pm0.03$      &        529 & D\\
NGC 2678 &$   -1.94\pm0.32 $&$   -2.00\pm0.28 $&$  -4.18\pm0.75 $&$   -5.34\pm0.57 $&$   8.29\pm0.55 $&$   6.10\pm0.43 $&$  -0.03\pm0.09 $&$   0.11\pm0.04$      &         16 & D\\
Teutsch 11 &$   -2.24\pm0.91 $&$   -2.61\pm0.87 $&$   0.30\pm1.28 $&$   -4.03\pm1.41 $&$   5.60\pm0.97 $&$   6.66\pm1.13 $&$   0.34\pm0.17 $&$   0.25\pm0.14$    &         16 & D\\
\hline
\multicolumn{11}{c}{Poor} \\ 
Berkeley 29 &$    0.56\pm0.45 $&$   -4.29\pm0.32 $&$   0.12\pm0.96 $&$   -6.46\pm0.88 $&$   7.43\pm0.79 $&$   6.26\pm0.68 $&$  -0.32\pm0.10 $&$   0.53\pm0.07$   &        137 & B\\
NGC 1663 &$    1.13\pm0.60 $&$   -1.32\pm0.72 $&$   3.97\pm0.65 $&$   -4.94\pm0.72 $&$   6.83\pm0.51 $&$   7.27\pm0.55 $&$  -0.14\pm0.08 $&$   0.23\pm0.07$      &         49 & B\\
NGC 2395 &$    1.22\pm0.38 $&$   -1.96\pm0.27 $&$   0.01\pm0.40 $&$   -4.32\pm0.48 $&$   5.80\pm0.31 $&$   7.17\pm0.36 $&$   0.01\pm0.06 $&$   0.27\pm0.05$      &        142 & B\\
Alessi 57 &$   -0.92\pm0.80 $&$   -7.89\pm0.68 $&$   1.11\pm1.36 $&$   -4.85\pm1.94 $&$   5.81\pm1.22 $&$   9.15\pm1.55 $&$  -0.01\pm0.19 $&$   0.30\pm0.14$     &         14 & C\\
Dias 8 &$   -4.51\pm0.48 $&$   -2.85\pm0.44 $&$  -1.13\pm1.62 $&$   -4.26\pm1.69 $&$   8.29\pm1.24 $&$   9.02\pm1.32 $&$   0.26\pm0.16 $&$   0.40\pm0.10$        &         30 & C\\
Ivanov 2 &$   -1.02\pm0.73 $&$    0.41\pm0.89 $&$  -0.89\pm0.98 $&$   -3.62\pm1.33 $&$   3.29\pm0.76 $&$   4.56\pm0.88 $&$  -0.46\pm0.21 $&$   0.22\pm0.18$      &         15 & C\\
NGC 7772 &$   17.50\pm0.57 $&$  -10.00\pm0.57 $&$   4.83\pm1.85 $&$   -8.49\pm1.63 $&$   7.59\pm1.33 $&$   6.63\pm1.21 $&$   0.13\pm0.23 $&$   0.09\pm0.06$      &          2 & C\\
DolDzim 2 &$    1.92\pm0.49 $&$   -3.25\pm0.59 $&$   3.30\pm0.92 $&$   -5.57\pm1.13 $&$   7.23\pm0.75 $&$   8.79\pm0.86 $&$  -0.05\pm0.11 $&$   0.48\pm0.07$     &         85 & D\\
DolDzim 7 &$   18.77\pm0.75 $&$  -12.13\pm0.70 $&$  -1.82\pm1.02 $&$   -5.70\pm1.23 $&$   5.79\pm0.80 $&$   7.56\pm0.94 $&$  -0.14\pm0.15 $&$   0.03\pm0.03$     &          1 & D\\
Dolidze 26 &$   -0.64\pm0.18 $&$   -2.24\pm0.25 $&$  -0.96\pm0.21 $&$   -4.13\pm0.24 $&$   6.17\pm0.17 $&$   6.84\pm0.19 $&$  -0.13\pm0.03 $&$   0.30\pm0.02$    &        536 & D\\
Dolidze 35 &$    3.87\pm0.36 $&$    0.85\pm0.37 $&$   0.32\pm0.78 $&$   -5.61\pm0.77 $&$   7.11\pm0.57 $&$   6.22\pm0.56 $&$   0.23\pm0.09 $&$   0.18\pm0.06$    &         28 & D\\
Juchert 1 &$   -0.61\pm0.69 $&$    0.95\pm0.70 $&$   4.88\pm0.77 $&$    2.17\pm1.50 $&$   1.46\pm0.72 $&$   5.75\pm1.25 $&$   0.41\pm0.17 $&$   0.17\pm0.13$     &          4 & D\\
Kronberger 13 &$    5.79\pm1.57 $&$   -5.39\pm1.57 $&$  -7.12\pm5.16 $&$    4.26\pm4.65 $&$   8.24\pm3.87 $&$   7.52\pm3.68 $&$   0.53\pm0.43 $&$   0.70\pm0.15$ &          9 & D\\
NGC 2224 &$    0.66\pm0.22 $&$   -0.91\pm0.16 $&$   0.63\pm0.16 $&$   -3.16\pm0.20 $&$   4.24\pm0.13 $&$   5.47\pm0.15 $&$  -0.14\pm0.03 $&$   0.19\pm0.02$      &        252 & D\\
NGC 2234 &$    0.14\pm0.07 $&$   -3.65\pm0.07 $&$   0.40\pm0.16 $&$   -5.88\pm0.18 $&$   5.48\pm0.13 $&$   6.11\pm0.14 $&$  -0.06\pm0.03 $&$   0.36\pm0.02$      &       2221 & D\\
NGC 2265 &$    1.60\pm0.16 $&$   -2.27\pm0.19 $&$   1.26\pm0.31 $&$   -3.82\pm0.36 $&$   4.61\pm0.25 $&$   5.24\pm0.28 $&$  -0.12\pm0.06 $&$   0.31\pm0.04$      &        149 & D\\
NGC 6525 &$   -2.39\pm0.51 $&$   -3.05\pm0.49 $&$   0.00\pm0.55 $&$   -2.63\pm0.75 $&$   5.56\pm0.45 $&$   8.24\pm0.61 $&$   0.06\pm0.08 $&$   0.21\pm0.06$      &         41 & D\\
NGC 6738 &$    1.51\pm0.17 $&$   -2.69\pm0.17 $&$  -0.36\pm0.23 $&$   -3.93\pm0.24 $&$   6.44\pm0.19 $&$   6.71\pm0.20 $&$   0.22\pm0.03 $&$   0.18\pm0.02$      &        255 & D\\
NGC 6837 &$  -23.18\pm2.77 $&$   -4.49\pm2.88 $&$  -0.13\pm0.66 $&$   -3.63\pm0.57 $&$   5.60\pm0.55 $&$   4.48\pm0.50 $&$   0.39\pm0.09 $&$   0.02\pm0.01$      &          5 & D\\
\hline
NGC 6839 &$    0.11\pm0.66 $&$   -4.88\pm0.57 $&$  -0.05\pm0.57 $&$   -6.04\pm0.54 $&$   7.48\pm0.48 $&$   7.12\pm0.46 $&$   0.12\pm0.06 $&$   0.29\pm0.05$      &        116 & D\\
NGC 6840 &$    1.08\pm0.61 $&$   -2.49\pm0.58 $&$   0.24\pm0.47 $&$   -6.07\pm0.51 $&$   6.20\pm0.41 $&$   6.34\pm0.40 $&$   0.06\pm0.06 $&$   0.24\pm0.06$      &         91 & D\\
NGC 6843 &$    3.26\pm0.68 $&$   -1.61\pm0.66 $&$   0.70\pm0.51 $&$   -4.69\pm0.55 $&$   5.72\pm0.44 $&$   6.24\pm0.46 $&$   0.13\pm0.07 $&$   0.14\pm0.07$      &         33 & D\\
NGC 6858 &$   -0.27\pm0.43 $&$   -3.35\pm0.34 $&$   0.46\pm0.42 $&$   -4.43\pm0.43 $&$   7.27\pm0.33 $&$   7.71\pm0.35 $&$   0.14\pm0.05 $&$   0.36\pm0.04$      &        261 & D\\
NGC 6950 &$   -0.89\pm0.34 $&$   -6.36\pm0.39 $&$  -0.01\pm0.27 $&$   -6.38\pm0.27 $&$   6.44\pm0.21 $&$   6.72\pm0.22 $&$   0.42\pm0.03 $&$   0.09\pm0.03$      &         80 & D\\
NGC 7084 &$   -5.50\pm0.51 $&$  -12.09\pm0.52 $&$  -0.04\pm0.47 $&$   -9.43\pm0.43 $&$   7.43\pm0.32 $&$   7.31\pm0.33 $&$   0.29\pm0.05 $&$   0.19\pm0.04$      &         97 & D\\
Riddle 15 &$    2.73\pm0.90 $&$   -8.10\pm0.88 $&$  -2.42\pm3.10 $&$   -2.21\pm4.75 $&$   7.27\pm2.27 $&$  11.87\pm3.67 $&$   0.76\pm0.18 $&$   0.24\pm0.15$     &          3 & D\\
Teutsch 12 &$    0.81\pm0.37 $&$   -1.98\pm0.35 $&$  -0.60\pm0.79 $&$   -2.89\pm0.96 $&$   4.97\pm0.63 $&$   6.22\pm0.78 $&$  -0.08\pm0.13 $&$   0.31\pm0.09$    &         29 & D\\
\hline
\end{tabular}
\tablefoot {The {\it c} subscripts indicate the parameters for the clusters, while the {\it f}~subscripts indicate the fields ones. The correlation coefficient~($\rho_f$), mixture proportion~($n_c$) and estimated number of members~($n_{\rm memb}$) are adimensionals, whereas all the other parameters are in mas~yr$^{-1}$~units. The ``Class'' column is the same as in Table~\ref{table:1}. The solutions are divided following their visual classifications.}
\end{table}