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     -1.80343     0.102433     0.134404
    0.400000     -2.10752     0.101904     0.134143
     1.00000     -2.38171     0.173990     0.296018
 
log10(M*[h^-2 M_sun]) > 10.25
    0.100000     -2.51148     0.104875     0.138750
    0.400000     -2.68871     0.156997     0.249925
     1.00000     -2.86200     0.166824     0.275766
     2.00000     -3.62600     0.226057     0.504285

log10(M*[h^-2 M_sun]) > 10.75
     0.100000     -3.50930    0.0978012     0.126428
     0.400000     -3.55753     0.190485     0.351342
      1.00000     -3.61682     0.201206     0.393114
      2.00000     -4.59453     0.262409     0.812666