; K-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)
   0.00893970      10.6054    -0.518942  3.19174e+08
  0.000440161    0.0241160    0.0673468  8.24984e+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   0.00000000   0.00000000   0.00000000
   8.81250000   0.00000000   0.00000000   0.00000000
   8.93750000   0.00000000   0.00000000   0.00000000
   9.06250000   0.00000000   0.00000000   0.00000000
   9.18750000   0.00000000   0.00000000   0.00000000
   9.31250000   0.00000000   0.00000000   0.00000000
   9.43750000   0.01124288   0.00733482   0.01515094
   9.56250000   0.00519958   0.00257913   0.00782003
   9.68750000   0.00592115   0.00373128   0.00811102
   9.81250000   0.00756930   0.00581277   0.00932582
   9.93750000   0.00707740   0.00573092   0.00842389
  10.06250000   0.00681215   0.00571536   0.00790894
  10.18750000   0.01016867   0.00890796   0.01142938
  10.31250000   0.00972339   0.00882488   0.01062189
  10.43750000   0.00781474   0.00718517   0.00844431
  10.56250000   0.00764439   0.00720679   0.00808199
  10.68750000   0.00808565   0.00766077   0.00851053
  10.81250000   0.00558036   0.00527042   0.00589029
  10.93750000   0.00307523   0.00283593   0.00331453
  11.06250000   0.00171278   0.00156654   0.00185901
  11.18750000   0.00073447   0.00064776   0.00082117
  11.31250000   0.00031281   0.00027986   0.00034575
  11.43750000   0.00013211   0.00010613   0.00015809