Figure 4

Evolution of Infrared Luminosity functions of Galaxies in the AKARI NEP-Deep field: Revealing the cosmic star formation history hidden by dust

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

Dataset details

Source label: Figure 4

Contributor: Shengdong Lu

Files: Goto_10_Fig_4.tsv

Short description: 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

Paper link: https://arxiv.org/abs/1001.0013