\begin{table}%t5
%\centering
\par
\caption{\label{revisedcen}The revised SBF distance estimates for the Centaurus cluster galaxies, based on the SBF-measurements from Mieske \& Hilker (\cite{Mieske03b}). The first six columns correspond to Table~4 from Mieske \& Hilker (\cite{Mieske03b}). The revised columns are those of the newly calculated $\Delta {\rm sim}$, $\Delta BG$, $\Delta GC$, and hence $\overline{m}_{ I}$, $(m-M)$ and linear distance $d$. We report a typo from Mieske \& Hilker (\cite{Mieske03b}): the colour of CCC 75 is $(V-I)=1.02$~mag, not 1.12~mag.}
\begin{tabular}{rrrrrrrrrrrr}\hline\hline
Nr. & Field & $P_0$ [ADU] & $P_1$ [ADU]& $ZP$ & $S/N$ & $\Delta {\rm sim}$ & $\Delta BG$ & $\Delta GC$ & $\overline{m}_{ I}$ & $(m-M)$ & $d$ [Mpc]\\\hline
N4696 & 1 & 2.33 $\pm$ 0.04 & 0.488 &  32.78 &  4.78 & 0.090 & 0.090 &0.23& 31.840 $\pm$ 0.120 &33.14 $\pm$ 0.17 &  42.5 $\pm$   3.20 \\
  75 & 1,2 & 3.30 $\pm$ 0.35 & 0.86 &  32.77 &  3.84 & 0.178 & 0.079 &0.18 &  31.289 $\pm$ 0.430 &33.60 $\pm$ 0.45 &   52.5 $\pm$    11.0  \\
  61 & 1 & 2.94 $\pm$ 0.25 & 0.51 &  32.76 &  5.76 & 0.174 & 0.068 &0.26 &  31.456 $\pm$ 0.290 &33.23 $\pm$ 0.32 &   44.2 $\pm$   6.50\\ 
  70 & 1 & 3.56 $\pm$ 0.20 & 0.32 &  32.76 &  11.1 &  0.20 & 0.012 &0.34 &   31.260 $\pm$ 0.310 &32.58 $\pm$ 0.33 &  32.8 $\pm$   5.10\\
  52 & 1 & 2.81 $\pm$ 0.33 & 0.64 &  32.76 &  4.39 & 0.168 & 0.072 &0.22 &  31.473 $\pm$ 0.430 &33.47 $\pm$ 0.45 &  49.4 $\pm$    10.0\\  
  89 & 2 & 2.16 $\pm$ 0.13 & 0.29 &  32.78 &  7.45 & 0.150 & 0.020 &0.25 &  31.772 $\pm$ 0.290 & 33.50 $\pm$ 0.31 &  50.1 $\pm$   7.30  \\
N4709 & 3 & 1.90 $\pm$ 0.10 & 0.38 &  32.67 &   5.00 & 0.140 & 0.089 &0.06 &  31.623 $\pm$ 0.083 & 32.50 $\pm$ 0.15 & 31.6 $\pm$   2.20 \\
 124 & 3 & 6.28 $\pm$ 1.28 & 3.36 &  32.67 &  1.87 & 0.153 & 0.199 &0.13 &  30.561 $\pm$ 0.430 &  33.33 $\pm$ 0.57 &  46.3 $\pm$    12.0 \\
 123 & 3 & 5.38 $\pm$ 0.43 & 0.62 &  32.67 &  8.68 & 0.151 & 0.041 &0.19 &  30.594 $\pm$ 0.430 & 32.86 $\pm$ 0.45 &  37.3 $\pm$   7.70\\  
 121 & 3 & 2.65 $\pm$ 0.50 & 0.76 &  32.67 &  3.49 & 0.183 & 0.116 &0.24 &  31.454 $\pm$ 0.460 & 33.54 $\pm$ 0.47 &  51.1 $\pm$    11.0\\
 115 & 3 & 4.02 $\pm$ 0.59 & 1.34 &  32.67 &  3.00 & 0.145 & 0.169 &0.17 &  31.063 $\pm$ 0.430 & 33.49 $\pm$ 0.45 &  50.0 $\pm$    10.0\\  
 111 & 3 & 6.02 $\pm$ 0.28 & 0.46 &  32.67 &  13.1 & 0.122 & 0.035 &0.18 &  30.527 $\pm$ 0.280 & 32.88 $\pm$ 0.30 &  37.7 $\pm$   5.30\\  
 125 & 4 & 5.28 $\pm$ 0.94 & 0.47 &  32.78 &  11.2 & 0.166 & 0.028 &0.65 &  31.198 $\pm$ 0.380 & 33.24 $\pm$ 0.40 &  44.5 $\pm$   8.30\\  
  58 & 5 & 2.62 $\pm$ 0.24 & 0.92 &  32.72 &  2.85 & 0.184 & 0.096 &0.13 &  31.419 $\pm$ 0.430 &33.73 $\pm$ 0.44 &  55.7 $\pm$    11.0\\   
  68 & 6 & 5.03 $\pm$ 1.49 & 4.13 &  32.72 &  1.22 & 0.144 & 0.396 &0.13 &  31.058 $\pm$ 0.430 & 33.62 $\pm$ 0.47 &  53.1 $\pm$    12.0\\\hline
& & & & & & & & &  &    {\bf 33.28 $\pm$ 0.09} & {\bf 45.3 $\pm$ 2.0}\\\hline
\end{tabular}
\end{table}