**Table 4:** Observed and total stellar mass density in the K20 survey, as a function of redshift. Reference value are given for the BF estimates; lower errors take into account the Poisson noise and the uncertainties in the mass estimates. Upper limits have been computed with respect to the values provided by the MA method, to provide an estimate of the global uncertainties.
$\begin{table} \par \begin{displaymath} \begin{array}{l\vert ccc} \hline\hline... ... value is actually a lower limit: see text for detail. \end{list}\par\end{table}$

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