; G-band derived colour selected late-type 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)
   0.00272888      10.5892     -1.44658  1.70267e+08
  0.000238098    0.0266404    0.0296940  4.31054e+06
; Then we present the V/V_max data points; x   phi  phi-1sig  phi+1sig
   8.56250000   0.05902331   0.04211422   0.07593240
   8.68750000   0.05060687   0.04221142   0.05900232
   8.81250000   0.03816551   0.03269534   0.04363567
   8.93750000   0.03456124   0.03055966   0.03856282
   9.06250000   0.03129275   0.02898807   0.03359743
   9.18750000   0.02486904   0.02221915   0.02751893
   9.31250000   0.02179631   0.01997892   0.02361370
   9.43750000   0.02151120   0.01967285   0.02334954
   9.56250000   0.01491044   0.01369303   0.01612784
   9.68750000   0.01408459   0.01298947   0.01517971
   9.81250000   0.01095662   0.01004516   0.01186808
   9.93750000   0.00911698   0.00846760   0.00976635
  10.06250000   0.00773829   0.00723264   0.00824394
  10.18750000   0.00576330   0.00540984   0.00611675
  10.31250000   0.00511340   0.00483170   0.00539509
  10.43750000   0.00426560   0.00405947   0.00447173
  10.56250000   0.00242944   0.00230619   0.00255269
  10.68750000   0.00183804   0.00170194   0.00197414
  10.81250000   0.00101048   0.00089795   0.00112301
  10.93750000   0.00043087   0.00038491   0.00047682
  11.06250000   0.00017916   0.00015720   0.00020113
  11.18750000   0.00006432   0.00004406   0.00008457
  11.31250000   0.00000000   0.00000000   0.00000000
  11.43750000   0.00000661   0.00000071   0.00001427