Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands and the UK) and with the participation of ISAS and NASA.

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Tables 7 to 13 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/372/364

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... K-correction

K-correction is defined as the ratio: $\frac{L(\nu ')}{L(\nu)}$ where $L(\nu)$ is the luminosity at frequency $\nu$ , and $\nu = (1+z) \nu '$ . Thus, $K(z) = \frac{L(\nu \times [1 + z])}{L(\nu)}\cdot$

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