\begin{table}%t1
  \caption{The sample of observed early-type galaxies from the K20 survey.	\label{sample}}
%\begin{center}
{  \begin{tabular}{c c c c c c c c c c c c}
  \hline\hline
  \noalign{\smallskip}
  K20 name & $z$ & $R$ & $R-K_{\rm s}$ & $n$ & $K_V$ & $R_{\rm e}$ & $\langle\mu^B\rangle_{\rm e}$ & $\sigma$ & {\it EW}[OII] & $M_B$ & $\log{{{\cal M}_{{\rm K}_{\rm V}}}\over{\cal M_{\odot}}}$\\
  & & & & & & kpc & mag/arcsec$^2$ & km~s$^{-1}$ & \AA & & \\
  \hline
  CDFS\_00060 & 1.188  & 24.89 & 5.56 & & & & & & &\\
  CDFS\_00369 & 0.8930 & 23.30 & 4.14 & 1.85~$\pm$~0.39 & 7.37~$\pm$~0.18 & 0.84~$\pm$~0.05 & 17.78~$\pm$~0.15 & 119~$\pm$~21 & 9.0~$\pm$~1.1 & --20.41& 10.31~$\pm$~0.15\\
  CDFS\_00467 & 0.8956 & 22.90 & 4.63 & 3.45~$\pm$~0.39 & 5.72~$\pm$~0.25 & 1.52~$\pm$~0.10 & 18.40~$\pm$~0.15 & 140~$\pm$~18 & 4.3~$\pm$~0.8 & --21.09& 10.58~$\pm$~0.11\\
  CDFS\_00468 & 1.019  & 24.86 & 5.03 & & & & & &&\\
  CDFS\_00532 & 1.2115 & 23.92 & 5.22 & 2.04~$\pm$~0.33 & 6.82~$\pm$~0.20 & 1.41~$\pm$~0.10 & 17.43~$\pm$~0.16 & 260~$\pm$~30 & 2.5~$\pm$~0.5 & --21.89& 11.16~$\pm$~0.10\\
  CDFS\_00547 & 1.2243 & 23.68 & 5.07 & 1.90~$\pm$~0.31 & 7.50~$\pm$~0.14 & 0.74~$\pm$~0.04 & 16.15~$\pm$~0.14 & 256~$\pm$~28 & 2.3~$\pm$~0.4 & --21.76& 10.93~$\pm$~0.10\\
  CDFS\_00571 & 0.9551 & 22.33 & 4.79 & 5.00~$\pm$~0.15 & 3.83~$\pm$~0.02 & 6.81~$\pm$~0.48 & 20.65~$\pm$~0.16 & 182~$\pm$~21 & 3.7~$\pm$~0.5 & --22.08& 11.23~$\pm$~0.10\\
  CDFS\_00590 & 1.2235 & 24.35 & 5.28 & 4.98~$\pm$~0.25 & 4.03~$\pm$~0.12 & 4.09~$\pm$~0.52 & 20.54~$\pm$~0.29 & 119~$\pm$~49 & 4.1~$\pm$~1.1 & --21.09& 10.68~$\pm$~0.36\\
  CDFS\_00633 & 1.0963 & 22.43 & 5.49 & 4.78~$\pm$~0.21 & 4.00~$\pm$~0.12 & 6.65~$\pm$~0.12 & 19.97~$\pm$~0.05 & 260~$\pm$~23 & $<$$1.4$ & --22.71& 11.55~$\pm$~0.08\\
  CDFS\_00354 & 0.6672 & 22.01 & 4.07 & 3.58~$\pm$~0.28 & 5.20~$\pm$~0.20 & 3.08~$\pm$~0.12 & 20.39~$\pm$~0.09 & 99~$\pm$~19 & 2.6~$\pm$~0.6$^*$ & --20.61 & 10.52~$\pm$~0.17\\
  \\
  q0055\_00028 & 1.0524 & 24.19 & 5.09 & 0.8~$\pm$~0.8 & 7.17~$\pm$~0.48 & 1.17~$\pm$~0.65 & 18.08~$\pm$~1.22 & 227~$\pm$~30 & $<$$3.6$ & --20.82 & 10.99~$\pm$~0.26\\
  q0055\_00068 & 1.1043 & 23.53 & 5.18 & 4.3~$\pm$~1.0 & 4.55~$\pm$~0.73 & 3.60~$\pm$~1.00 & 19.75~$\pm$~0.61 & 84~$\pm$~31 & 2.3~$\pm$~0.7 & --21.60 & 10.37~$\pm$~0.34\\
  q0055\_00114 & 0.8891 & 23.48 & 4.33 & 2.0~$\pm$~2.0 & 6.71~$\pm$~1.78 & 2.43~$\pm$~0.74 & 19.99~$\pm$~0.66 & 52~$\pm$~22 & $<$$2.1$ & --20.50 & 9.98~$\pm$~0.38\\
  q0055\_00123 & 0.9270 & 22.96 & 4.84 & 3.8~$\pm$~1.0 & 5.69~$\pm$~0.67 & 1.23~$\pm$~0.40 & 17.62~$\pm$~0.71 & 186~$\pm$~19 & 1.6~$\pm$~0.5 & --21.39 & 10.74~$\pm$~0.16\\
  q0055\_00247 & 0.931  & 24.43 & 4.54 & & & & & & $<$$2.8$ & &\\
  q0055\_00295 & 1.1680 & 23.75 & 5.59 & 4.8~$\pm$~0.3 & 4.35~$\pm$~0.20 & 2.67~$\pm$~0.70 & 18.93~$\pm$~0.57 & 170~$\pm$~28 & $<$$1.4$ & --21.77 & 10.85~$\pm$~0.18\\
  q0055\_00318 & 0.8962 & 23.87 & 5.07 & 4.5~$\pm$~1.1 & 5.17~$\pm$~0.70 & 1.26~$\pm$~0.57 & 18.87~$\pm$~0.99 & 105~$\pm$~30 & $<$$0.8$$^*$ & --20.20 & 10.21~$\pm$~0.31\\
  q0055\_00331 & 0.8980 & 22.95 & 5.09 & 4.9~$\pm$~0.3 & 4.15~$\pm$~0.19 & 3.83~$\pm$~0.77 & 20.08~$\pm$~0.44 & 216~$\pm$~46 & $<$$0.8$$^*$ & --21.40 & 11.18~$\pm$~0.19\\
  q0055\_00338 & 0.9324 & 23.12 & 4.96 & 2.8~$\pm$~0.6 & 5.93~$\pm$~0.50 & 2.41~$\pm$~0.43 & 19.23~$\pm$~0.39 & 113~$\pm$~19 & $<$$2.5$ & --21.24 & 10.59~$\pm$~0.16\\
  q0055\_00169 & 0.6699 & 22.70 & 4.23 & 1.3~$\pm$~0.8 & 7.15~$\pm$~0.62 & 1.64~$\pm$~0.36 & 19.50~$\pm$~0.47 & 90~$\pm$~19 & $<$$0.9$$^*$ & --20.14 & 10.32~$\pm$~0.20\\
  \hline
  \end{tabular}}  
  \parbox{16.5cm}{
 $^*$ For [OIII]5007. }
%\end{center}
\par
\end{table}