\begin{table}%t3
  \caption{Results from the fitting. The fitting regions and signal-to-noise 
    per pixel in the continuum is listed. Best-fit  velocity dispersions 
    normalized to the same physical aperture
    ($r_{\rm ap} = 0.595~h^{-1}$~kpc) and their confidence intervals are shown. 
    "AGN cont.'' indicates that there is too much AGN~contamination 
    in the spectrum to obtain a~reliable fit.}\label{table:t4}
\small%\centerline
{
\begin{tabular}{llrlll|lrlll}
\hline\hline
          & Fitting region& {\it S/N} & $\sigma_{*}$ & 68\% CI & 95\% CI & Fitting region & {\it S/N} & $\sigma_{*}$ & 68\% CI & 95\% CI \\
          &    {\AA} &    &     km~s$^{-1}$ &   km~s$^{-1}$  &  km~s$^{-1}$ & {\AA} &  & km~s$^{-1}$ & km~s$^{-1}$ & km~s$^{-1}$ \\
\hline		
3C 20     & AGN cont.     & 4  & ... & ... & ... 
          & too noisy     & 1  & ... & ... & ... \\
3C 28     & AGN cont.     & 6  & ... & ... & ...
          & too noisy     & 1  & ... & ... & ... \\
3C 31 & 5220--5650 & 25 & 247 & [246, 251] & [244, 252] & 4000--4500 & 7 & 260 & [255, 266] & [248, 273] \\
3C 33 & 5220--5420 & 11 & 188 & [178, 199] & [168, 210] & AGN cont.  & 6 & ... & ... & ... \\
3C 35 & 5090--5390 & 6 & 224 & [215, 233] & [206, 243] & 3800--4250 & 3 & 206 & [191, 224] & [176, 242] \\
3C 66B$^{{a}}$ & poor fit  & 18 & ... & ... &  ... & 4000--4470 & 6 & 165 & [155, 174] & [146, 185] \\
3C 76.1 & 5220--5560 & 18 & 193 & [188, 198] & [183, 203] & 4000--4470 & 7 & 192 & [174, 209] & [157, 225] \\
3C 98 &  5220--5570 & 17 & 136 & [128, 143] & [120, 152] & 4000--4420 & 7 & 159 & [149, 170] & [140, 181] \\
3C 388 & 5150--5740 & 15 & 232 & [211, 243] & [195, 259] & too noisy & 2 & ... & ... & ... \\
3C 381 & 5100--5410 & 9 & 221 & [212, 231] & [202, 241] & too noisy & 1 & ... & ... & ... \\
3C 401 & 5100--5230 & 5 & 136 & [95, 166] & [65, 284] & too noisy & 1 & ... & ... & ... \\
3C 433 & 5220--5700 & 10 & 128 & [121, 131] & [115, 136] & too noisy & 1 & ... & ... & ... \\
3C 442A & 5100--5590 & 15 & 198 & [188, 208] &  [193, 203] & 4000-4450 & 6 & 216 & [207, 225] & [198, 234] \\
3C 449 & 5100--5650 & 17 &  263 & [258, 267] & [254, 271] & 3800--4500 & 6 & 192 & [187, 198] & [181, 204] \\
3C 452 & 5120--5310 & 7 &  289 & [284, 296] & [274, 307] & AGN cont. & 4 & ... & ... & ... \\
3C 465 & 5220--5570 & 19 &  338 & [332, 344] & [326, 350] &  4000--4400 & 7 & 362 & [351, 375] & [340, 388] \\
4C 11.71 & 5220--5600 & 8 &  227 & [224, 232] & [220, 234] & 4000--4450 & 6 & 250 & [242, 259] & [234, 267] \\
4C 12.03 & 5100--5420 & 8 &  245 & [231, 257] & [219, 271] & too noisy & 1 & ... & ... & ... \\  
4C 35.40 & 5220--5570 & 16 & 205 & [198, 205] & [190, 213] & 4000--4420 & 6 & 193 & [184, 200] & [176, 209] \\
\hline
\end{tabular}}
\medskip
$^{{a}}$ Despite good signal-to-noise in the red part,
  for unknown reasons, an acceptable fit could not be obtained.
\end{table}