The VISCACHA survey -- deep and resolved photometry of star clusters in
  the Magellanic Clouds
  The VISCACHA (VIsible Soar photometry of star Clusters in tApii and Coxi
HuguA\footnote{LMC and SMC names in the Tupi-Guarani language spoken by native
people in Brazil}) Survey is an ongoing project based on deep and
spatiallyresolved photometric observations of Magellanic Cloud star clusters,
collected using the SOuthern Astrophysical Research (SOAR) telescope together
with the SOAR Adaptive Module Imager. So far we have used $>$300h of telescope
time to observe $\sim$150 star clusters, mostly with low mass ($M < 10^4
M_{\odot}$) on the outskirts of the LMC and SMC. With this high-quality data
set, we homogeneously determine physical properties using deep colour-magnitude
diagrams (ages, metallicities, reddening, distances, mass, luminosity and mass
functions) and structural parameters (radial density profiles, sizes) for these
clusters which are used as a proxy to investigate the interplay between the
Magellanic Clouds and their evolution. We present the VISCACHA survey and its
initial results, based on our first two papers. The project's long term goals
and expected legacy to the community are also addressed.
