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The HerMES submillimetre local and low-redshift luminosity functions

Marchetti M. V. L., Franceschini V. A. A., Aussel M. B. H., Bock A. B. J. J., Buat D. B. V., Clements A. C. D. L. et al. | 2015

arXiv | ADS | Publisher page

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Figure 15

Marchetti_16_Fig_15_64rows.tsv | 64 rows | 3232 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

The HerMES submillimetre local and low-redshift luminosity functions

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Figure 15

Discussion