  The main goal of this study is to compile a catalogue including the
fundamental parameters of a complete sample of 277 star clusters (SCs) of the
Large Magellanic Cloud (LMC) observed in the Washington photometric system,
including 82 clusters very recently studied by us. All the clusters' parameters
such as radii, deprojected distances, reddenings, ages and metallicities have
been obtained by appyling essentially the same procedures which are briefly
described here. We have used empirical cumulative distribution functions to
examine age, metallicity and deprojected distance distributions for different
cluster subsamples of the catalogue. Our new sample made up of 82 additional
clusters recently studied by us represents about a 40% increase in the total
number of LMC SCs observed up to now in the Washington photometric system. In
particular, we report here the fundamental parameters obtained for the first
time for 42 of these clusters. We found that single LMC SCs are typically older
than multiple SCs. Both single and multiple SCs exhibit asymmetrical
distributions in log (age). We compared cluster ages derived through isochrone
fittings obtained using different models of the Padova group. Although $t_G$
and $t_B$ ages obtained using isochrones from Girardi et al. (2002) and Bressan
et al. (2012), respectively, are consistent in general terms, we found that
$t_B$ values are not only typically larger than $t_G$ ages but also that
Bressan et al.'s age uncertainties are clearly smaller than the corresponding
Girardi et al. values.
