Table 1
Cosmological model dependence of the galaxy luminosity function: far-infrared results in the LemaƮtre-Tolman-Bondi model
Columns: x_value = log10 luminosity in Lsun x_upper_error/x_lower_error = asymmetric x errors in dex y_value = log10 Phi in Mpc^-3 dex^-1 y_upper_error/y_lower_error = asymmetric y errors in dex redshift = redshift bin center upper_redshift_error/lower_redshift_error = redshift bin half-widths is_upper_limit/is_lower_limit = limit flags