- Table 1:
Parameters used for the library of template SEDs.
- Table 2:
Average M*/LR ratios as a function of redshift and
spectral type, computed in the mass complete-sample, as defined by
the thick solid curve of Fig. 1. All refers to all
galaxies in the K20 sample, including also those with photometric redshift
only. Early refer to early and early+emission
spectroscopic types and late to late spectroscopic types, as
defined in Sect. 2. Only objects with spectroscopic redshift are
included in the last two columns. M*/L ratio in the V and K bands are available
in electronic form at the web site http://www.arcetri.astro.it/~k20
- Table 3:
Best fit Schechter parameters of the Galaxy Stellar Mass
Functions in the K20 survey. Errors indicate
levels. Parameters without error have been fixed to the best fit value
of the lower z bin.
- 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.