\begin{table}%t4
\caption{\label{table4}Results of the Bulge-disk decomposition.}
\small%\centerline
 {
\begin{tabular}{lcccccccccc}
\hline\hline
&&&&&&&&&& \\[-8pt]
Object & Morph. type & \multicolumn{2}{c}{de Vaucouleurs bulge} & \multicolumn{3}{c}{Sersic bulge} & $B/T_{\rm deV}$ & $B/T_{\rm S}$ & $\Delta$ $B/T$ & $\Delta \chi ^2_\nu$ \\
     & type & bulge & disk & bulge & bar & disk & & & & \\
     & & $m_{R}$ & $m_{R}$ & $m_{R}$ & $m_{R}$ & $m_{R}$ & & & & \\
\hline
RR143\_09192 & SB0 & 19.10 & 17.33 & 17.31 & 20.70 & 18.55 & 0.16 & 0.77 & --0.6 & 30.6\\
RR143\_24246 & S0 &18.36 & 17.37 & 18.47 & ... & 17.51 & 0.29 & 0.29 & --0.01 & 0.9\\
RR210\_11372 & dE & ... & 17.58 & ... & ... & 17.58 & 0.00 & 0.00 & 0 & 0.36\\
RR210\_13493 & SB0 & 15.11 & 14.87 & 16.18 & 17.30 & 14.53 & 0.44 & 0.23 & 0.22 & 10.6\\
RR216\_03519 & dE & 21.95 & 17.29 & 20.69 & ... & 17.32 & 0.01 & 0.04 & --0.03 & 0.1\\
RR216\_04052 & SB0 & 17.95 & 14.67 & 17.39 & ... & 14.70 & 0.05 & 0.08 & --0.03 & 1.5\\
RR216\_12209 & Sc & 22.07 & 15.63 & 21.79 & ... & 15.63 & 0.00 & 0.00 & 0 & 0.1\\
RR242\_08064 & dE & 19.25 & 18.18 & 19.28 & ... & 18.30 & 0.27 & 0.29 & --0.02 & 0.3\\
RR242\_13326 & S0 & 17.17 & 16.54 & 18.64 & ... & 16.29 & 0.36 & 0.10 & 0.26 & 0.1\\
RR242\_15689 & dE & 19.52 & 18.10 & 20.93 & ... & 17.95 & 0.21 & 0.06 & 0.15 & 0.3\\
RR242\_20075 & dE & 17.39 & 16.79 & 18.74 & ... & 16.53 & 0.37 & 0.12 & 0.25 & 0.8 \\
RR242\_23187 & S & ... & ... & 17.63 & ... & 17.96 & ... & 0.57 & ... & ... \\
RR242\_22327 & SB0 & 16.72 & 15.51 & 17.58 & 16.56 & 15.79 & 0.25 & 0.41 & --0.16 & 2.2\\
RR242\_24352 & SB0 & 14.59 & 14.52 & 15.31 & 17.36 & 14.17 & 0.49 & 0.29 & 0.2 & 21.4\\
RR242\_25575 & SB? & 16.27 & 17.70 & 17.62 & ... & 16.77 & 0.79 & 0.31 & 0.47 & 0.8\\
RR242\_28727 & dE & 18.25 & 17.38 & 17.95 & ... & 17.40 & 0.31 & 0.38 & --0.07 & --82.9\\
RR242\_36267 & dE & 21.31 & 17.92 & 23.06 & ... & 17.89 & 0.04 & 0.01 & 0.03 & 22.5 \\
\hline
\end{tabular}}
\medskip
Notes: bulge and disk magnitudes and bulge-to-total light ($B/T$) ratios of the fit with de~Vaucouleurs bulges (Cols.~3,~4) and Sersic bulges (Cols.~5$-$7) respectively. Columns~8$-$10 give the Bulge-to-Total light ratios of the two models respectively and their difference. The last column gives the difference between the~$\chi ^2_\nu$ of the de~Vaucouleurs and the Sersic-model~fit.
\end{table}