Tables 1 and 2 are also 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/435/521

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The VLA and VLBA are operated by the National Radio Astronomy Observatory, a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.

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... cookbook

Available online at www.nrao.edu

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...

Measurement errors were not considered when running the statistical tests.

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...

Here we use the highest resolution radio flux, instead of a "matched'' linear-resolution flux. The latter flux is dominated by extra-nuclear (non-AGN related) emission for these lowest luminosity AGNs and is thus not directly comparable to the radio fluxes of the other more luminous radio sources used in the RLF computation.

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...

Ho et al. (2003a) list 54 nuclei with H $\alpha$ luminosity upper limits; of these, the nucleus of NGC 4494 shows other emission lines and was classified as a (highly uncertain) "LINER 2'' by Ho et al. (1997a).

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