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Studies of IRAS sources at high galactic latitudes - III. Luminosity functions at 25, 60 and 100 mu.m and the correlation of optical and infrared luminosities.

Rowan-Robinson M., Helou G., Walker D. | 1987

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Fig. 4(a)

Rowan_Robinson_87_Fig_4_a_44rows.tsv | 44 rows | 2043 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

Studies of IRAS sources at high galactic latitudes - III. Luminosity functions at 25, 60 and 100 mu.m and the correlation of optical and infrared luminosities.

Dataset entries

Fig. 4(a)

Discussion