Article record

Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to <i>z</i> ∼ 6

Koprowski M. P., Wijesekera J. V., Dunlop J. S., Lisiecki K., McLeod D. J., McLure R. J. et al. | 2026

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Table 3

Koprowski_26_Table_3.tsv | 24 rows | 1389 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

Evolution of the infrared luminosity function and its corresponding dust-obscured star formation rate density out to <i>z</i> ∼ 6

Dataset entries

Table 3

Discussion