Table 6: Summary of the derived parameters of the LF parameters obtained by various authors by fitting them with Schechter functions, in several rest-frame bands, in different redshift bins, and from different samples of field galaxies.
Source Limit Area Band z $M^{\ast}-5\log h_{70}$ $\phi ^{\ast }$ $\alpha $
  [mag] $\left[{\rm deg}^{2}\right]$     [AB] $\left[10^{-3}h_{70}^{3}~{\rm Mpc}^{-3}\right]$  
Kochanek et al. (2001) K < 11.25 <7000 K 0.02 $-22.36\pm0.05$ $3.97\pm0.34$ $-1.09\pm0.06$
Arnouts et al. (2007) F( $3.6~\mu{\rm m})>9~\mu$Jy 0.85 K 0.50 $-22.83\pm0.30$ $3.47\pm1.4$ $-1.1\pm0.2$
Arnouts et al. (2007) F(3.6  $\mu {\rm m})>9~\mu$Jy 0.85 K 0.90 $-23.12\pm0.08$ $4.00\pm0.3$ $-1.11\pm0.06$
Arnouts et al. (2007) F(3.6  $\mu {\rm m})>9~\mu$Jy 0.85 K 1.35 $-23.13\pm0.17$ $2.60\pm0.5$ $-1.1\pm0.2$
Arnouts et al. (2007) F(3.6  $\mu m)>9~\mu$Jy 0.85 K 1.75 $-23.28\pm0.14$ $1.62\pm0.3$ $-1.1\pm0.2$
Feulner et al. (2003) K< 17.50 0.18 J 0.30..0.60 $-22.93\pm0.24$ $2.60\pm0.80$ -1.00 fixed
Dahlen et al. (2005)   0.036 J 0.75..1.00 $-23.09\pm^{0.24}_{0.22}$ $1.97\pm^{0.60}_{0.40}$ $-1.31\pm^{0.10}_{0.09}$
Gabasch et al. (2006) I(AB)<26.8 0.01 z 0.4 $-22.78\pm0.41$ $2.7\pm1.2$ -1.33(fixed)
Gabasch et al. (2006) I(AB)<26.8 0.01 z 0.9 $-22.93\pm0.44$ $2.2\pm0.7$ -1.33(fixed)
Gabasch et al. (2006) I(AB)<26.8 0.01 z 1.32 $-23.05\pm0.48$ $1.9\pm0.5$ -1.33(fixed)
Gabasch et al. (2006) I(AB)<26.8 0.01 z 1.31..1.91 $-22.71\pm0.18$ $2.0\pm0.3$ -1.33(fixed)
Gabasch et al. (2006) I(AB)<26.8 0.01 z 1.89 $-23.14\pm0.51$ $1.70\pm0.4$ -1.33(fixed)
Gabasch et al. (2006) I(AB)<26.8 0.01 i 0.4 $-22.58\pm0.31$ $2.7\pm1.3$ -1.33(fixed)
Gabasch et al. (2006) I(AB)<26.8 0.01 i 0.9 $-22.69\pm0.34$ $2.2\pm0.8$ -1.33(fixed)
Gabasch et al. (2006) I(AB)<26.8 0.01 i 1.32 $-23.78\pm0.37$ $1.9\pm0.5$ -1.33(fixed)
Gabasch et al. (2006) I(AB) < 26.8 0.01 i 1.89 $-22.85\pm0.40$ $1.7\pm0.4$ -1.33(fixed)
Gabasch et al. (2006) I(AB) < 26.8 0.01 i 1.91..2.61 $-22.93\pm0.14$ $1.9\pm0.2$ -1.33(fixed)
Marchesini et al. (2007) K<23(max) 0.65 R 2.0..2.5 $-22.67\pm^{0.20}_{0.22}$ $1.07\pm^{0.27}_{0.27}$ $-1.01\pm^{0.21}_{0.20}$


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