  Aims: We present a new method that uses luminosity or stellar mass functions
combined with clustering measurements to select samples of galaxies at
different redshifts likely to follow a progenitor-to-descendant relationship.
As the method uses clustering information, we refer to galaxy samples selected
this way as clustering-selected samples. We apply this method to infer the
number of mergers during the evolution of MUSYC early-type galaxies (ETGs) from
z~1 to the present-day. Methods: The method consists in using clustering
information to infer the typical dark-matter halo mass of the hosts of the
selected progenitor galaxies. Using LambdaCDM predictions, it is then possible
to follow these haloes to a later time where the sample of descendants will be
that with the clustering of these descendant haloes. Results: This technique
shows that ETGs at a given redshift evolve into brighter galaxies at lower
redshifts (considering rest-frame, passively evolved optical luminosities).
This indicates that the stellar mass of these galaxies increases with time and
that, in principle, a stellar mass selection at different redshifts does not
provide samples of galaxies in a progenitor-descendant relationship.
Conclusions: The comparison between high redshift ETGs and their likely
descendants at z=0 points to a higher number density for the progenitors by a
factor 5.5+-4.0, implying the need for mergers to decrease their number density
by today. Because the luminosity densities of progenitors and descendants are
consistent, our results show no need for significant star-formation in ETGs
since z=1, which indicates that the needed mergers are dry, i.e. gas free.
