\begin{table}%t12
\caption{\label{WDana}Wilson-Devinney analysis, as obtained on the basis of both photometry and spectroscopy.}             
%\centering
\par
\begin{tabular}{l l l l l l l l l}      
\hline\hline  \noalign{\smallskip}
Object & Model & $T_{\rm eff}^{\rm S} / T_{\rm eff}^{\rm P}$ & $\Omega_{\rm P}$ & $\Omega_{\rm S}$ &
$(L_{\rm S}/L_{\rm P})_{B}$ & $(L_{\rm S}/L_{\rm P})_{V}$ & $(L_{\rm S}/L_{\rm P})_{I}$ & $(L_{\rm S}/L_{\rm P})_B^{{\rm sp}}$ \\ 
  &  & & & & $\ell_{3,B}$ & $\ell_{3,V}$ & $\ell_{3,I}$ &  \\
\hline                    
  4 110409 & sd &  $0.654 \pm0.007$  & $5.732\pm0.092$  & $2.922$ (fixed)  & $1.292\pm0.023$ & $1.353\pm0.024$ &  $1.367\pm0.024$ & $1.392\pm0.036$ \\
  4 113853 & sd &  $0.737 \pm0.015$  & $3.868\pm0.090$  & $3.209$ (fixed)  & $0.680\pm0.010$ & $0.713\pm0.009$ &  $0.753\pm0.009$ & $0.681\pm0.058$ \\
  4 117831 & d  &  $0.981 \pm0.023$  & $4.855$ (fixed)  & $4.479\pm0.108$  & $1.175\pm0.052$ & $1.177\pm0.050$ &  $1.180\pm0.049$ & $1.009\pm0.103$ \\
  4 121084 & d  &  $0.940 \pm0.007$  & $3.770$ (fixed)  & $3.817\pm0.043$  & $0.707\pm0.061$ & $0.713\pm0.010$ &  $0.720\pm0.010$ & $0.704\pm0.061$ \\
  4 121110 & d  &  $0.894 \pm0.007$  & $3.820\pm0.035$  & $4.184\pm0.059$  & $0.424\pm0.005$ & $0.433\pm0.005$ &  $0.442\pm0.005$ & $0.415\pm0.047$ \\
  4 121461 & d  &  $0.949 \pm0.023$  & $6.980\pm0.133$  & $6.822\pm0.099$  & $0.907\pm0.030$ & $0.914\pm0.029$ &  $0.923\pm0.029$ & $0.954\pm0.063$ \\
  4 159928 & sd &  $0.723 \pm0.010$  & $3.138\pm0.024$  & $2.983$ (fixed)  & $0.357\pm0.003$ & $0.376\pm0.003$ &  $0.397\pm0.004$ & $0.453\pm0.029$ \\
  4 160094 & d  &  $0.854 \pm0.018$  & $5.517$ (fixed)  & $5.545\pm0.100$  & $0.476\pm0.050$ & $0.489\pm0.007$ &  $0.502\pm0.007$ & $0.428\pm0.101$ \\
  4 163552 & d  &  $0.997 \pm0.004$  & $3.983\pm0.026$  & $4.214\pm0.044$  & $0.798\pm0.024$ & $0.799\pm0.016$ &  $0.800\pm0.014$ & $0.926\pm0.171$ \\
  	   &    &   		  &		     &		           & $0.142\pm0.014$ & $0.112\pm0.012$ &  $0.119\pm0.006$ &                 \\
  4 175149 & sd &  $0.849 \pm0.006$  & $4.411\pm0.056$  & $3.171$ (fixed)  & $1.176\pm0.025$ & $1.200\pm0.023$ &  $1.229\pm0.023$ & $1.415\pm0.132$ \\
  4 175333 & d  &  $0.879 \pm0.022$  & $5.054\pm0.151$  & $5.010\pm0.196$  & $0.582\pm0.034$ & $0.595\pm0.035$ &  $0.609\pm0.036$ & $0.562\pm0.103$ \\
  5 016658 & d  &  $1.007 \pm0.009$  & $4.086$ (fixed)  & $4.590\pm0.068$  & $0.609\pm0.074$ & $0.612\pm0.008$ &  $0.614\pm0.008$ & $0.604\pm0.074$ \\
  5 026631 & sd &  $0.734 \pm0.007$  & $3.507\pm0.030$  & $3.226$ (fixed)  & $0.495\pm0.003$ & $0.519\pm0.003$ &  $0.547\pm0.003$ & $0.736\pm0.049$ \\
  5 032412 & d  &  $0.880 \pm0.008$  & $7.284$ (fixed)  & $6.949\pm0.073$  & $0.578\pm0.050$ & $0.584\pm0.007$ &  $0.583\pm0.007$ & $0.546\pm0.005$ \\
  5 038089 & d  &  $1.012 \pm0.009$  & $4.606\pm0.047$  & $5.065\pm0.067$  & $0.693\pm0.019$ & $0.692\pm0.018$ &  $0.691\pm0.018$ & $0.678\pm0.032$ \\
  5 095337 & d &   $0.936 \pm0.007$  & $3.685\pm0.022$  & $3.835\pm0.040$  & $0.676\pm0.008$ & $0.684\pm0.008$ &  $0.691\pm0.008$ & $0.659\pm0.085$ \\
  5 095557 & d  &  $0.908 \pm0.013$  & $5.991\pm0.107$  & $6.602\pm0.165$  & $0.523\pm0.015$ & $0.532\pm0.015$ &  $0.541\pm0.015$ & $0.625\pm0.190$ \\
  5 100485 & d  &  $1.008 \pm0.007$  & $5.193\pm0.076$  & $5.216\pm0.080$  & $0.966\pm0.034$ & $0.965\pm0.034$ &  $0.963\pm0.034$ & $0.930\pm0.052$ \\
  5 100731 & c  &  $0.828 \pm0.035$  & $3.851\pm0.058$  & $3.351$ (fixed)  & $0.517\pm0.014$ & $0.533\pm0.013$ &  $0.552\pm0.012$ & $0.438\pm0.041$ \\
  5 106039 & sd &  $0.638 \pm0.006$  & $5.178\pm0.057$  & $2.928$ (fixed)  & $1.007\pm0.009$ & $1.076\pm0.009$ &  $1.168\pm0.009$ & $1.062\pm0.063$ \\
  5 111649 & d  &  $1.025 \pm0.011$  & $4.600$ (fixed)  & $4.736\pm0.067$  & $0.889\pm0.056$ & $0.886\pm0.015$ &  $0.882\pm0.014$ & $0.880\pm0.052$ \\
  5 123390 & d  &  $1.017 \pm0.020$  & $5.077$ (fixed)  & $5.631\pm0.106$  & $0.587\pm0.060$ & $0.587\pm0.011$ &  $0.585\pm0.010$ & $0.584\pm0.061$ \\
  5 180185 & d  &  $1.036 \pm0.029$  & $7.724\pm0.169$  & $8.571\pm0.249$  & $0.707\pm0.042$ & $0.705\pm0.025$ &  $0.700\pm0.024$ & $0.611\pm0.042$ \\
  5 180576 & d  &  $0.813 \pm0.027$  & $4.918\pm0.170$  & $5.071\pm0.207$  & $0.450\pm0.027$ & $0.465\pm0.028$ &  $0.483\pm0.029$ & $0.45 \pm0.07 $ \\
  5 185408 & d  &  $0.944 \pm0.018$  & $5.052$ (fixed)  & $4.957\pm0.094$  & $0.757\pm0.047$ & $0.764\pm0.017$ &  $0.772\pm0.016$ & $0.619\pm0.045$ \\
  5 196565 & d  &  $0.867 \pm0.016$  &$5.956$ (fixed)&$6.639\pm0.120$&$0.43 \pm0.04$\tablefootmark{a}&\tablefootmark{b}&$0.453\pm0.009$ & $0.413\pm0.040$ \\
  5 261267 & sd &  $0.728 \pm0.004$  & $3.353\pm0.013$  & $2.923$ (fixed)  & $0.439\pm0.002$ & $0.461\pm0.003$ &  $0.487\pm0.001$ & $0.451\pm0.039$ \\
  5 265970 & d  &  $0.901 \pm0.012$  & $4.157$ (fixed)  & $5.370\pm0.056$  & $0.219\pm0.024$ & $0.264\pm0.001$ &  $0.227\pm0.001$ & $0.233\pm0.024$ \\
  5 266015 & sd &  $0.757 \pm0.005$  & $3.512\pm0.026$  & $2.759$ (fixed)  & $0.494\pm0.002$ & $0.515\pm0.002$ &  $0.539\pm0.002$ & $0.617\pm0.045$ \\
  5 266131 & d  &  $0.936 \pm0.007$  & $4.510$ (fixed)  & $4.727\pm0.065$  & $0.647\pm0.060$ & $0.655\pm0.008$ &  $0.661\pm0.007$ & $0.644\pm0.060$ \\
  5 266513 & d  &  $0.959 \pm0.018$  & $4.390$ (fixed)  & $4.530\pm0.084$  & $0.692\pm0.070$ & $0.697\pm0.016$ &  $0.703\pm0.015$ & $0.733\pm0.076$ \\
  5 277080 & sd &  $0.685 \pm0.004$  & $3.932\pm0.047$  & $2.884$ (fixed)  & $0.567\pm0.015$ & $0.600\pm0.008$ &  $0.641\pm0.008$ & $0.690\pm0.022$ \\
  5 283079 & d  &  $0.997 \pm0.010$  & $5.162$ (fixed)  & $5.184\pm0.074$  & $0.987\pm0.086$ & $0.987\pm0.015$ &  $0.988\pm0.015$ & $0.936\pm0.088$ \\
\hline                  
\end{tabular}
\tablefoot {Listed parameters: system type (detached, semi-detached or contact), temperature ratio, normalized surface potentials and passband luminosity ratios. Third light contribution is given for
the system 4~163552 (normalized to total flux at phase~0.25). The given potentials and the luminosity ratios are those obtained \textit{including} the spectroscopic constraints (final WD/PHOEBE analysis).\\
\tablefoottext{a}{$B$ data missing, ratio given by the WD code on the basis of the $I$~data, via the atmosphere models;} 
\tablefoottext{b}{$V$ data missing.}}
\end{table}