\begin{table}%t2
\caption{\label{all_res}Summary of results; the age, distance modulus, reddening
and thus the distance from the Sun was derived by fitting isochrones
to the $\Delta a$~photometry. $R_{V}$ was set to 3.1. For the distance of the Sun from
the galactic center, a value of 8.5~kpc was used, the Trumpler classification was taken 
from Lyng{\aa} (\cite{Lyng1987}) and the errors in the final digits of the corresponding quantity
are given in parenthesis. Questionable peculiar stars are marked by asterisks (see the 
corresponding cluster result section for details). All photometric values are in units of mmags.}
\small
%\centering
\par
\begin{tabular}{lllll}
\hline\hline\noalign{\smallskip}
Name & Berkeley~11 & Berkeley~94 & Haffner~15 & Lyng{\aa}~1 \\
     & \object{C0417+448} & \object{C2220+556} & \object{C0743$-$326} & \object{C1356$-$619} \\
\hline
$l/b$ & 157.08/$-$3.64 & 103.13/$-$1.18 & 247.94/$-$4.16 & 310.86/$-$0.35\\
$E(B-V)$ ($\pm$0.05) & 0.95 & 0.65 & 1.10 & 0.50 \\
$m_V - M_V$ ($\pm$0.2) & 15.2 & 14.6 & 15.1 & 13.0 \\
$d$~[kpc] & 2.82(46) & 3.29(54) & 2.21(36) & 1.95(32) \\
$R_{GC}$~[kpc] & 11.15(44) & 9.79(30) & 9.55(21) & 7.37(15) \\
$|z|$~[pc] & 179(29) & 68(11) & 160(26) & 12(2) \\
log~$t$ ($\pm$0.1) & 8.0 & 7.0 & 7.2 & 8.0  \\
Tr-type & II 2 m & II 3 p & II 2 m & II 2 p\\
$n$(member) & 54 & 77 & 83 & 40 \\
$n$(none) & 12 & 38 & 246 & 126 \\   
CP~No. (Webda):  & *25(322): +91/+123/+911      & 27($-$): $-$54/$-$/+2737  & 109(3): +45/$-$214/$-$3078  & 8(58): +48/+371/+3153  \\
                                $\Delta$a/$(B-V)_0$/$M_V$  & 38(188): +45/$-$84/$-$631   & 67(4): +42/$-$/+696    & 190($-$): +65/$-$129/1867     &  15(53): +26/+280/+2880 \\
                                 $[$mmag$]$ & 50(128): +42/$-$146/$-$2000 & 114($-$): +88/$-$/+1719    &                    & 22(56): $-$44/+498/+3016\\
                                  & *54(255): +111/+109/+384     &               &                    &  81(80): $-$25/+448/+3710 \\
                                  & 64(313): +33/$-$130/$-$1390  &              &                    & *82(40): +51/+187/+1510  \\
                                  &                     &              &                    & 93(57): +22/+307/+3132  \\
                                  &                     &              &                    & 103(52): +37/+253/+2801  \\
                                  &                     &              &                    & 105(24): $-$35/+130/+1089  \\
                                  &                     &              &                    & 109(125): $-$23/+512/+4570  \\
                                  &                     &              &                    & 111(87): $-$21/+523/+3909  \\
                                  &                     &              &                    & 112(85): +22/+388/+3912 \\
                                  &                     &              &                    & 127(31): $-$43/+143/+1556  \\
                                  &                     &              &                    & 134(67): $-$41/+420/+3378  \\
$n$(frames) & 30  & 24  & 34  & 30  \\
\hline 
Name & NGC~6031 & NGC~6405 & NGC~6834 & Ruprecht~130 \\
     & \object{C1603$-$539} & \object{C1736$-$321} & \object{C1950+292} & \object{C1744$-$301} \\
\hline
$l/b$ & 329.29/$-$1.55 & 356.62/$-$0.74 & 65.71/+1.19 & 359.21/$-$0.98\\
$E(B-V)$ ($\pm$0.05) & 0.50 & 0.20  & 0.70 & 1.20 \\
$m_V - M_V$ ($\pm$0.2) & 12.45  & 8.9 & 13.6 & 15.0  \\
$d$~[kpc] & 1.51(25) & 0.45(7) & 1.93(32) & 1.80(30)  \\
$R_{GC}$~[kpc] & 7.24(20) & 8.05(7) & 7.90(6) & 6.70(30) \\
$|z|$~[pc] & 41(7) & 6(1) & 40(7) & 31(5) \\
log~$t$ ($\pm$0.1) & 8.2 & 8.0 & 7.9 & 7.9  \\
Tr-type & I 3 p & II 3 r & II 2 m & II 1 p \\
$n$(member) & 67 & 134 & 201 & 140 \\
$n$(none) & 176 & 33 & 107 & 155 \\
CP~No. (Webda):      & 29(85): +28/+151/+2651  & *33(7): +32/+57/+1915  & 8(128): $-$82/+30/+1854  & 71($-$): +35/+83/$-$285  \\	
$\Delta$a/$(B-V)_0$/$M_V$    & 35(73): +20/+24/+1034    & 65(19): +55/$-$90/+839  & *32(125): $-$42/+771/$-$2637 & 79(1): +33/$-$187/$-$169   \\	
$[$mmag$]$                         & 69(70): $-$29/+387/+3017    & 135(77): +85/$-$94/+357  & *129(1): $-$46/+196/$-$3158  & 92(7): +48/$-$102/$-$518  \\	
                             & 199(54): $-$23/+583/+2893  &      & 137($-$): +41/$-$64/+1706  & 227($-$): +48/$-$72/+1157   \\	
                             &                            &      & 139(412): +36/$-$31/+2797  & 250(108): +60/$-$345/$-$2997  \\	
                             &                            &      & 198(67): $-$78/+97/$-$1128 &             \\	
                             &                            &      & 202(42): $-$59/$-$68/+526 &             \\	
                             &                            &      & 234(55): $-$57/$-$34/$-$385 &             \\	
                             &                            &      & 294(155): $-$71/$-$124/+1739 &             \\	
                             &                            &      & 297(73): $-$72/$-$35/$-$1963 &             \\	
$n$(frames) & 30  & 24  & 41  & 30  \\
\hline
\end{tabular}
\end{table}