Table 4: Evolution rates and zero-points for the amplitudes $\phi _0$and $\phi ^*$ of the Gaussian and Schechter components of the late-type luminosity function in the ESO-Sculptor Survey, as derived from the number-counts in the Johnson B, V and Cousins $R_{\rm c}$bands.
  ( $\Omega_{\rm m}$,  $\Omega_\Lambda)=(0.3$, 0.7) ( $\Omega_{\rm m}$,  $\Omega_\Lambda)=(1.0$, 0.0)
   P0.15    $\phi_0(0.15)$    $\phi^*(0.15)$   $\gamma$   $\phi_0(0)$   $\phi^*(0)$   P0.15    $\phi_0(0.15)$    $\phi^*(0.15)$   $\gamma$   $\phi_0(0)$   $\phi^*(0)$ 
$R_{\rm c}$   2.2   0.00252   0.02732   1.8   0.00211   0.02292   4.6   0.00320   0.03470   2.5   0.00287   0.03119 
V   4.3   0.00216   0.02347   2.5   0.00186   0.02019   5.7   0.00322   0.03493   2.8   0.00283   0.03072 
B   3.3   0.00267   0.02899   2.2   0.00226   0.02449   5.0   0.00355   0.03857   2.6   0.00313   0.03399 
Note:
-
The listed values of $\phi _0$ and $\phi ^*$ are in units of  h3 Mpc-3 mag-1, and are obtained with  H0 = 100 h km s-1 Mpc-1.
-
The linear, power-law parameterization of the evolution in $\phi _0$ and $\phi ^*$is defined in Eqs. (20) and (22) respectively.
-
Each value of $\phi ^*$ is related to the corresponding value of $\phi _0$ by the ratio  $\phi_0/0.4\ln10\;\phi^*=0.1$ (see Table 1).

Source LaTeX | All tables | In the text