# i-band LF from GAMA data, using L_sun assuming M_solar = 4.56
# as per Figure 10 of Baldry et al. 2012, MNRAS, 421, 621.
# number density is per dex per Mpc^3; assuming H0=70 km/s/Mpc.
# log luminosity, bin width, number density, error, number in sample.
 6.40   0.40     0.0212646     0.0204898     3
 6.80   0.40     0.0573008     0.0356729     7
 7.10   0.20     0.0456110     0.0186165    11
 7.30   0.20     0.0218301    0.00763824     9
 7.50   0.20     0.0402218     0.0114686    17
 7.70   0.20     0.0405885    0.00800396    34
 7.90   0.20     0.0329597    0.00619136    51
 8.10   0.20     0.0255299    0.00333634    89
 8.30   0.20     0.0296317    0.00257179   173
 8.50   0.20     0.0251609    0.00168645   249
 8.70   0.20     0.0219154    0.00123300   365
 8.90   0.20     0.0185911   0.000914956   526
 9.10   0.20     0.0155926   0.000656793   685
 9.30   0.20     0.0132215   0.000635115   597
 9.50   0.20     0.0101320   0.000465559   477
 9.70   0.20    0.00861542   0.000428500   406
 9.90   0.20    0.00824996   0.000417755   390
10.10   0.20    0.00708557   0.000387127   335
10.30   0.20    0.00636001   0.000372237   298
10.50   0.20    0.00490700   0.000322161   232
10.70   0.20    0.00281308   0.000243925   133
10.90   0.20    0.00171323   0.000190359    81
11.10   0.20   0.000401867   9.21946e-05    19
11.30   0.20   6.34533e-05   3.66348e-05     3
11.50   0.20       0.00000   3.00000e-05     0
11.70   0.20       0.00000   3.00000e-05     0