... function

Based on observations obtained at Canada-France-Hawaii Telescope.

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...

Full Table 3 is 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/400/891

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... 1997

Prior to 1997, mass function estimates were based on strongly contaminated samples of brown dwarf candidates.

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... error

Using the lower limit of $r_{\rm c}=1.3\hbox{$^\circ$ }$ for the cluster core radius in the susbtellar domain would yield $\alpha=0.63\pm0.11$ instead.

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... Database

Available at http://cfa-www.harvard.edu/stauffer/opencl/

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... boundary

We do not attempt to correct the observed Pleiades mass function for unresolved binaries in the substellar domain because the brown dwarf binary statistics is still very poorly known, as is the statistics of brown dwarfs companions to low mass stars

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