; K-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)
   0.00710279      10.4839    -0.944617  2.10136e+08
  0.000590091    0.0294251    0.0805289  9.04877e+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   0.01839248   0.00958909   0.02719587
   9.18750000   0.00000000   0.00000000   0.00000000
   9.31250000   0.00652316   0.00270998   0.01033635
   9.43750000   0.01538020   0.01114911   0.01961128
   9.56250000   0.01485340   0.01070353   0.01900328
   9.68750000   0.01562596   0.01168241   0.01956951
   9.81250000   0.01247445   0.00964983   0.01529907
   9.93750000   0.01117246   0.00895989   0.01338503
  10.06250000   0.01277256   0.01110040   0.01444472
  10.18750000   0.00953746   0.00819717   0.01087776
  10.31250000   0.00692298   0.00611748   0.00772849
  10.43750000   0.00611913   0.00540124   0.00683701
  10.56250000   0.00536667   0.00493361   0.00579974
  10.68750000   0.00364334   0.00338545   0.00390123
  10.81250000   0.00196174   0.00174197   0.00218151
  10.93750000   0.00094363   0.00083920   0.00104806
  11.06250000   0.00037654   0.00032592   0.00042717
  11.18750000   0.00012170   0.00009337   0.00015002
  11.31250000   0.00003702   0.00001974   0.00005431
  11.43750000   0.00001532   0.00000615   0.00002449