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Infrared luminosity functions based on 18 mid-infrared bands: revealing cosmic star formation history with AKARI and Hyper Suprime-Cam

Goto N. O. T., Utsumi R. M. Y., Matsuhara T. H. H., Toba Y. O. Y., Takagi C. Y. C. T., Kim E. K. E. S. J. et al. | 2019

arXiv | ADS | Publisher page

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Goto2019_Fig2_8um.tsv | 16 rows | 1314 bytes | TSV

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

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Goto2019_Fig3_12um.tsv | 14 rows | 1169 bytes | TSV

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

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Goto2019_Fig4_TIR.tsv | 20 rows | 1532 bytes | TSV

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

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