; G-band derived late-type c_r < 2.6 stellar mass function
; Schecter Function fit parameters
; phi* M* Alpha j  (next line formal errors)
; real errors are probably systematic: see Bell et al.\ 2003 for
; guidance (the errors depend on passband and/or stellar mass)
   0.00589508      10.5112     -1.26979  2.39633e+08
  0.000335132    0.0186434    0.0285373  3.90704e+06
; Then we present the V/V_max data points; x   phi  phi-1sig  phi+1sig
   8.56250000   0.06505574   0.04366534   0.08644613
   8.68750000   0.07320711   0.06460879   0.08180544
   8.81250000   0.04799416   0.04002676   0.05596155
   8.93750000   0.04443620   0.03823223   0.05064016
   9.06250000   0.03909315   0.03448391   0.04370239
   9.18750000   0.02870709   0.02537397   0.03204021
   9.31250000   0.02494731   0.02261295   0.02728167
   9.43750000   0.02676752   0.02445437   0.02908067
   9.56250000   0.01749840   0.01596177   0.01903503
   9.68750000   0.01817670   0.01706169   0.01929171
   9.81250000   0.01640520   0.01525517   0.01755523
   9.93750000   0.01427543   0.01337057   0.01518028
  10.06250000   0.01224849   0.01136685   0.01313014
  10.18750000   0.00938676   0.00879961   0.00997391
  10.31250000   0.00820031   0.00770407   0.00869654
  10.43750000   0.00669675   0.00630577   0.00708772
  10.56250000   0.00473231   0.00449669   0.00496792
  10.68750000   0.00292193   0.00273340   0.00311046
  10.81250000   0.00160139   0.00152450   0.00167828
  10.93750000   0.00070131   0.00064115   0.00076147
  11.06250000   0.00024135   0.00021772   0.00026499
  11.18750000   0.00006004   0.00004692   0.00007317
  11.31250000   0.00002254   0.00001216   0.00003293
  11.43750000   0.00000000   0.00000000   0.00000000