Table 3: Parameters of power-law fits to the projected-separation correlation function for other redshift surveys.
Survey Redshift range Absolute magnitude range Numb. r0 ( h-1 Mpc) $\gamma$ Reference
Galaxy type            
ESS $0.1\le z\le 0.51$\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 $ Pollo et al. (2006)
SDSS $z\le0.04$ $M_r{-}5\log h\le-18.0$ * 8730 $3.7 \pm0.3 $ $1.87\pm0.05$ Zehavi et al. (2005)
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.
ESS:            
- early-type galaxies $0.1\le z\le 0.51$ $M_{R_{\rm c}}{-}5\log h\le -16.0$ 218 $3.80\pm0.67$ $2.11\pm0.10$ present analysis
- late spiral galaxies $0.1\le z\le 0.51$ $M_{R_{\rm c}}{-}5\log h\le -16.0$ 279 $2.72\pm0.64$ $1.60\pm0.08$ id.
- dwarf galaxies $0.1\le z\le 0.51$ $M_{R_{\rm c}}{-}5\log h\le -16.0$ 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 $3.1 \pm0.8$ $2.4\pm0.3$ Meneux et al. (2006)
- 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 $6.05 \pm 0.35$ $1.94 \pm 0.03$ Madgwick et al. (2003)
- 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 $5.7 \pm 0.3$ $2.10 \pm 0.05$ Zehavi et al. (2005)
- 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 $6.59\pm0.17$ $1.96 \pm 0.05$ Budavári et al. (2003)
- blue $w(\theta)$   $-21\le M_r{-}5\log h$ 316 $4.51\pm0.19$ $1.68 \pm 0.09$ id.
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.

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