Astrophysical properties of star clusters in the Magellanic Clouds
  homogeneously estimated by $\texttt{ASteCA}$
  Aims. To produce an homogeneous catalog of astrophysical parameters of 239
resolved star clusters located in the Small and Large Magellanic Clouds,
observed in the Washington photometric system.
  Methods. The cluster sample was processed with the recently introduced
Automated Stellar Cluster Analysis ($\texttt{ASteCA}$) package, which ensures
both an automatized and a fully reproducible treatment, together with a
statistically based analysis of their fundamental parameters and associated
uncertainties. The fundamental parameters determined with this tool for each
cluster, via a color-magnitude diagram (CMD) analysis, are: metallicity, age,
reddening, distance modulus, and total mass.
  Results. We generated an homogeneous catalog of structural and fundamental
parameters for the studied cluster sample, and performed a detailed internal
error analysis along with a thorough comparison with values taken from
twenty-six published articles. We studied the distribution of cluster
fundamental parameters in both Clouds, and obtained their age-metallicity
relationships.
  Conclusions. The $\texttt{ASteCA}$ package can be applied to an unsupervised
determination of fundamental cluster parameters; a task of increasing relevance
as more data becomes available through upcoming surveys.
