\begin{table}%t3
%\centering
\par
%\begin{table}{
\small
\caption{Results of the host galaxy fitting for the de Vaucouleurs model.}
\label{globalprop}  
%\centering
\par
\begin{tabular}{lccclccccccccc}
\hline
\hline
Object          &  $z$  &$A_I$&$K_I$& $R^a$ &$m_{\rm core}$&$M_{\rm core}$& $m_{\rm host}$& $M_{\rm host}$ & $r_{\rm e}$ & $r_{\rm e}$ & $\mu_{\rm e}$& $\chi^2$ &
$\frac{\chi^2_{\rm deV.}}{\chi^2_{\exp}}$\\      
                &     &     &     & &              &      &              &      &[$''$]         & [kpc]        & [mag/sq$''$]   &     &    \\
\hline                                                                                                 PKS 0057--338   &0.875&0.04 &1.22 &E+&$19.65\pm0.04$&$-$24.78&$19.60\pm0.05$&$-$26.04&$0.34\pm0.06$&$ 3.54\pm0.21$&$16.66\pm0.18$& 4.97&1.09\\  
 S4 0218+35     &0.936$^b$&0.09 &1.50 &D&$19.42\pm0.05$&$-$25.25&$19.67\pm0.08$&$-$25.60&$0.51\pm0.03$&$4.79\pm0.28$&$17.76\pm0.20$& 2.09&0.77\\
 Q 0230+3429    &0.500&0.11 &0.45 &E+&$20.60\pm0.20$&$-$22.38&$15.61\pm0.06$&$-$27.82&$4.91\pm0.28$&$39.65\pm2.26$&$20.18\pm0.19$& 1.16&1.04\\ 
 PKS 0406+121   &0.504&1.09 &0.46 &N+&$19.29\pm0.04$&$-$24.69&$19.91\pm0.17$&$-$24.53&$0.54\pm0.03$&$4.38\pm0.24$&$18.64\pm0.29$& 0.96&0.99\\  
 PKS 0426--380   &1.111$^c$&0.06 &0.53 &D&$16.99\pm0.04$&$-$28.15&$20.25\pm0.12$&$-$23.50&$0.82\pm0.03$&$7.01\pm0.26$&$20.69\pm0.20$& 9.30&0.95\\  
 PKS 0754+100   &0.266&0.04 &0.21 &E&$15.51\pm0.03$&$-$25.82&$17.76\pm0.04$&$-$23.78&$2.46\pm0.21$&$13.45\pm1.15$&$21.83\pm0.27$&2.02&1.17 \\ 
 PKS 0820+225   &0.951&0.08 &1.46 &N+&$18.52\pm0.04$&$-$26.19&$20.67\pm0.10$&$-$25.50&$0.73\pm0.05$&$7.82\pm0.54$&$18.93\pm0.25$&1.20&1.00 \\ 
 PKS 0823+033   &0.506&0.18 &0.46 &U&$16.01\pm0.06$&$-$27.07&   $<$16.9    & $<$$-$26.6&             &              &              &8.23&     \\ 
 RX J0930.9+3933 &0.638&0.03 &0.66 &E+&$20.30\pm0.05$&$-$23.25&$18.92\pm0.04$&$-$25.28&$1.50\pm0.10$&$13.68\pm0.91$&$20.36\pm0.18$&1.10&1.35 \\ 
 B2 0937+26$^d$ &0.498&0.03 &0.45 &E+&              &      &$19.43\pm0.05$&$-$23.91&$0.85\pm0.13$&$6.84\pm1.08$&$20.23\pm0.39$&1.09&1.06 \\ 
 TXS 1040+244   &0.560&0.06 &0.53 &E+&$17.40\pm0.04$&$-$25.83&$18.60\pm0.06$&$-$25.16&$0.80\pm0.11$&$6.85\pm0.94$&$18.98\pm0.36$&1.84&1.12 \\ 
 1207+39W4      &0.615&0.06 &0.62 &E&$18.49\pm0.03$&$-$24.99&$18.92\pm0.09$&$-$25.17&$2.81\pm0.51$&$25.18\pm4.57$&$21.79\pm0.49$&1.87&1.04 \\ 
 Q 1214+1753    &0.679&0.07 &0.73 &N+&$17.13\pm0.03$&$-$26.62&$18.99\pm0.05$&$-$25.50&$1.12\pm0.22$&$10.50\pm2.06$&$19.57\pm0.48$&1.73&1.01 \\ 
 1ES 1249+174W  &0.644&0.04 &0.67 &U&$17.96\pm0.03$&$-$25.62&   $<$19.1    & $<$$-$25.2&             &              &              &2.18&     \\ 
 PKS 1349--439$^e$   &   ? &0.15 &     &U&$17.64\pm0.04$&$-$26.28&   $<$18.7    &         &             &              &              &1.58&     \\ 
 RX J1422.6+5801 &0.638&0.02 &0.66 &N+&$17.60\pm0.03$&$-$25.94&$18.86\pm0.08$&$-$25.33&$2.26\pm0.43$&$20.60\pm3.92$&$21.20\pm0.49$&1.62&1.00 \\ 
 TXS 1428+370   &0.564&0.02 &0.54 &E+&$21.36\pm0.60$&$-$21.85&$18.91\pm0.05$&$-$24.83&$0.38\pm0.04$&$3.27\pm0.34$&$17.70\pm0.28$&1.15&1.07 \\ 
 PKS 1519--273   &1.294&0.56 &2.58 &U&$17.88\pm0.04$&$-$28.21&   $<$18.1    & $<$$-$30.6&             &              &              &2.64&     \\ 
 OV $-$236        &0.352&0.30 &0.29 &E&$17.02\pm0.03$&$-$25.25&$18.31\pm0.03$&$-$24.25&$1.65\pm0.13$&$10.86\pm0.86$&$20.89\pm0.20$&10.06&1.36\\ 
 PKS 2029+121   &1.215&0.19 &2.28 &U&$18.33\pm0.04$&$-$27.20&   $<$19.9    & $<$$-$27.9&             &              &              &10.29&    \\  
 PKS 2131--021   &1.285&0.13 &2.24 &U&$18.64\pm0.04$&$-$27.00&   $<$19.9    & $<$$-$28.3 &             &              &              &1.69&     \\ 
 MH 2133--449$^e$&  ? &0.05 &     &N+&$18.86\pm0.03$&      &$21.28\pm0.09$& &$3.73\pm0.31$& & &1.65&0.99 \\ 
 PKS 2240--260   &0.774&0.05 &0.94 &U&$16.00\pm0.04$&$-$28.09&   $<$17.7     & $<$$-$27.3&             &              &              &4.98&     \\ 
 MS 2347.4+1924$^f$ &0.515&0.32 &0.47 &D&              &      &$18.85\pm0.04$&$-$24.89&$0.53\pm0.08$& $4.36\pm0.66$&$18.27\pm0.37$&1.37&0.93 \\ 
 \hline
\end{tabular}
\par
{$^a$ Code for galaxy detection and morphology class: U = unresolved, E = elliptical, D = disk, N = resolved, but unclassified, + new detection.}\\
{$^b$ Grav. lensed BL~Lac. $z = 0.96$ used for the core, $z = 0.685$ used for
the lensing galaxy.}\\
{$^c$ $z = 1.111$ used for the core, $z = 0.559$ used for the intervening galaxy. See subsection
\ref{notes} for details.}\\
{$^d$ Results given for $\epsilon = 0.28$, PA = 30\degr. See subsection
\ref{notes} for details.}\\
{$^e$ Observations taken through Cousins $R$-filter. Extinction and K-correction
  for corresponding filter used.}\\
{$^f$ Results given for $\epsilon = 0.44$, PA = 65\degr. See subsection
\ref{notes} for details.}
\end{table}