redshift / log10(integrated ND[h^3Mpc^-3]) / log10(integrated ND[h^3Mpc^-3])_err_up / log10(integrated ND[h^3Mpc^-3])_err_down

log10(M*[h^-2 M_sun]) > 9.00
     0.100000     -1.81167    0.0619133    0.0724885
     0.400000     -1.86209    0.0756772    0.0923479
      1.00000     -1.97233     0.126469     0.179968
      2.00000     -2.17243     0.137743     0.203716

log10(M*[h^-2 M_sun]) > 10.25
     0.100000     -3.00867     0.119301     0.165320
     0.400000     -3.01968     0.178726     0.317151
      1.00000     -3.18696     0.132090     0.196590
      2.00000     -3.28282     0.193525     0.365221
      3.00000     -3.65009     0.224108     0.492930

log10(M*[h^-2 M_sun]) > 10.75
     0.400000     -4.26583     0.263206     0.834312
      1.00000     -4.48239     0.243436     0.702773
      2.00000     -4.46429     0.222771     0.566281
      3.00000     -4.48222     0.252961     0.686049