Field Galaxy Luminosity Function (From EEP98). 

   L/L*       M-M*    N(>L)    f(>L)
----------------------------------------
   3.0       -1.19    0.056    0.043
   2.5       -0.99    0.108    0.072
   2.0       -0.75    0.215    0.120
   1.5       -0.44    0.446    0.201
   1.0        0.00    1.000    0.337
   0.5        0.75    2.643    0.571
   0.25       1.51    5.095    0.748
   0.10       2.50    9.265    0.884
   0.05       3.25    12.92    0.938
   0.01       5.0     22.56    0.985
   0.001      7.5     38.71    0.998
   0.0001    10.0     57.75    0.9994
   0.00001   12.5     80.13    0.99958
   0.000001  15.0     106.4    0.99960
---------------------------------------
                      N(<M)    f(<M)


Notes:

L/L* = luminosity relative to L*

M-M* = absolute magnitude relative to M_V* = -21.35

N(>L) = N(<M) = cumulative number of galaxies (normalized by volume)
                brighter than L (M_V)

f(>L) = f(<M) = fraction of the total luminosity contributed by all
                galaxies brighter than L, normalized to 1.0 for L=0.