\begin{table}%t3
\caption{Parameters of power-law fits to the projected-separation correlation function for other redshift surveys.}
\label{T3}
\small%\centerline
{
\begin{tabular}{llcrccl}
\hline
\hline
Survey & Redshift range & Absolute magnitude range & Numb. & $r_0$ (\hmpc) & $\gamma$ & Reference \\
Galaxy type & \\
\hline
ESS    & $0.1\le z\le0.51$\dag  & $M_{R_{\rm c}}{-}5\log h\le -16.0$ &     654 & $3.50\pm1.21$ & $1.93\pm0.09$ & present analysis\\
VVDS   & $0.1\le z\le0.5$       & $M_B{-}5\log h\le-17.0$               &   1089 & $3.0 \pm0.5 $ & $1.7 \pm0.1 $ & \citet{pollo06} \\
SDSS   & $z\le0.04$             & $M_r{-}5\log h\le-18.0$~*             &   8730 & $3.7 \pm0.3 $ & $1.87\pm0.05$ & \citet{zehavi05} \\
SDSS   & $z\le0.06$             & $M_r{-}5\log h\le-17.0$~*             &  23 560 & $4.6 \pm0.2 $ & $1.89\pm0.03$ & id. \\
2dFGRS & $0.01\le z\le0.20$     &                                     & 165 659 & $5.0 \pm0.3 $ & $1.70\pm0.03$ & id. \\
\hline
ESS: \\
- early-type galaxies    & $0.1\le z\le0.51$  &  $M_{R_{\rm c}}{-}5\log h\le -16.0$ &     218 & $3.80\pm0.67$ & $2.11\pm0.10$ & present analysis\\
- late spiral galaxies   & $0.1\le z\le0.51$  &  $M_{R_{\rm c}}{-}5\log h\le -16.0$ &     279 & $2.72\pm0.64$ & $1.60\pm0.08$ & id.\\
- dwarf galaxies         & $0.1\le z\le0.51$  &  $M_{R_{\rm c}}{-}5\log h\le -16.0$ &     159 & $1.85\pm0.83$ & $2.46\pm0.38$ & id.\\
VVDS: \\
- elliptical/S0 galaxies & $0.2\le z\le0.6$   & $M_{B_{AB}}{-}5\log h\le-15.0$         &     164 & $3.1 \pm0.8$    & $2.4\pm0.3$    & \citet{meneux06} \\
- Sb-Sc galaxies         & $0.2\le z\le0.6$   & $M_{B_{AB}}{-}5\log h\le-15.0$         &     736 & $2.8 \pm0.4$    & $1.9\pm0.2$    & id. \\
- Magellanic irregulars  & $0.2\le z\le0.6$   & $M_{B_{AB}}{-}5\log h\le-15.0$         &     507 & $1.7 \pm0.3$    & $1.8\pm0.1$     & id.  \\
2dFGRS: \\
- passive galaxies       & $0.01\le z\le0.20$ &                                      &  36 318 & $6.05 \pm 0.35$ & $1.94 \pm 0.03$ & \citet{madgwick03} \\
- active galaxies        & $0.01\le z\le0.20$ &                                      &  60 473 & $3.89 \pm 0.31$ & $1.55\pm 0.04$  & {id.} \\
SDSS: \\
- red  galaxies          & $0.03\le z\le0.07$ & $-20\le M_r{-}5\log h\le-19.0$~*       &   5804 & $5.7 \pm 0.3$   & $2.10 \pm 0.05$ & \citet{zehavi05} \\
- blue galaxies          & $0.03\le z\le0.07$ & $-20\le M_r{-}5\log h\le-19.0$~*       &   8419 & $3.6 \pm 0.3$   & $1.70 \pm 0.05$ & {id.} \\
SDSS: \\
- red  $w(\theta)$       &                    &   $-21\le M_r{-}5\log h$               &     343 & $6.59\pm0.17$   & $1.96 \pm 0.05$ & \citet{budavari03} \\
- blue $w(\theta)$       &                    &   $-21\le M_r{-}5\log h$               &     316 & $4.51\pm0.19$   & $1.68 \pm 0.09$ & {id.} \\
\hline
\end{tabular}}
\medskip
Notes: 
\dag\ The over-density in the interval $0.41<z<0.44$ is excluded from the listed redshift interval. 
$^*$ The star symbol in the absolute magnitude range column indicates
that the corresponding sample is volume limited to the quoted absolute
magnitude limits. Elsewhere, the indicated absolute magnitude results
from the combination of the apparent magnitude and redshift limits of
the sample.
\end{table}