Table 1: Parameters of the Gaussian and Schechter components of the composite luminosity functions fitted to the ESO-Sculptor spectral-type luminosity functions, in the $R_{\rm c}$, V, and B filters.
Sample Numb. Morphol. Gaussian component Schechter component  $\phi _0$ 
  of gal. content   $M_0-5\log h$   $\Sigma_a$   $\Sigma_b$    $M^*-5\log h$   $\alpha$    $\overline{0.4 \ln10\; \phi^*}$ 
early-type galaxies
$R_{\rm c}\le 21.5$  291 E+S0+Sa   $-20.87\pm0.23$    $0.84\pm0.24$    $1.37\pm0.36$       
$V\le 21.0$  156 E+S0+Sa  -20.37   0.84   1.37       
$B\le 22.0$  108 E+S0+Sa  -19.47   0.84   1.37       
intermediate-type galaxies
$R_{\rm c}\le 21.5$  270 Sb+Sc/dSph   $-20.27\pm0.21$    $0.91\pm0.18$      $-19.28\pm0.37$    $-1.53\pm0.33$   0.83 
$V\le 21.0$  169 Sb+Sc/dSph  -19.87   0.91     -18.88   -1.53   0.83 
$B\le 22.0$  154 Sb+Sc/dSph  -19.27   0.91     -18.28   -1.53   0.83 
late-type galaxies
$R_{\rm c}\le 21.5$  309 Sc+Sd/dI   $-19.16\pm0.29$    $0.97\pm0.13$      $-18.12\pm0.22$   -0.30   0.1 
$V\le 21.0$  168 Sc+Sd/dI  -18.76   0.97     -17.72   -0.30   0.1 
$B\le 22.0$  190 Sc+Sd/dI  -18.36   0.97     -17.32   -0.30   0.1 
Notes:
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For the 2-component luminosity functions fitted to the intermediate-type and late-type galaxies, the morphological content of the 2 components appear separated by a "/''.
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The listed luminosity function parameters correspond to  H0 = 100 h km s-1 Mpc-1,  $\Omega _{\rm m}=0.3$, and  $\Omega _\Lambda =0.7$.

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