; G-band derived early-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)
   0.00825791      10.6241    -0.603046  3.08388e+08
  0.000379453    0.0189848    0.0421599  5.83002e+06
; Then we present the V/V_max data points; x   phi  phi-1sig  phi+1sig
   8.56250000   0.00000000   0.00000000   0.00000000
   8.68750000   0.00667967   0.00362801   0.00973134
   8.81250000   0.00649383   0.00456846   0.00841919
   8.93750000   0.00461768   0.00239745   0.00683791
   9.06250000   0.01247259   0.00892733   0.01601786
   9.18750000   0.00758070   0.00502756   0.01013385
   9.31250000   0.00596654   0.00441749   0.00751559
   9.43750000   0.00828318   0.00687603   0.00969033
   9.56250000   0.00684744   0.00546722   0.00822765
   9.68750000   0.00592456   0.00482618   0.00702295
   9.81250000   0.00732197   0.00645074   0.00819320
   9.93750000   0.00736595   0.00649160   0.00824030
  10.06250000   0.00765030   0.00686537   0.00843523
  10.18750000   0.00796450   0.00738066   0.00854834
  10.31250000   0.00838559   0.00779765   0.00897353
  10.43750000   0.00836144   0.00797958   0.00874331
  10.56250000   0.00854907   0.00801331   0.00908483
  10.68750000   0.00712799   0.00683916   0.00741682
  10.81250000   0.00511594   0.00485922   0.00537266
  10.93750000   0.00308215   0.00295760   0.00320671
  11.06250000   0.00163955   0.00151645   0.00176266
  11.18750000   0.00075187   0.00069708   0.00080667
  11.31250000   0.00031649   0.00027459   0.00035839
  11.43750000   0.00011093   0.00009184   0.00013002