The VISCACHA survey - deep and resolved photometry of star clusters in the Magellanic Clouds(póster presentado, proceeding aceptado).

BRUNO DIAS; FRANCISCO MAIA; LEANDRO KERBER; JOAO F. C. DOS SANTOS JR.; EDUARDO BICA; TINA ARMOND; BEATRIZ BARBUY; LUCIANO FRAGA; JOSE A. HERNANDEZ-JIMENEZ; ORLANDO J. KATIME SANTRICH; RAPHAEL A. P. OLIVEIRA; ANGELES PEREZ-VILLEGAS; ANDRÉS E. PIATTI; BRUNO QUINT; DAVID SANMARTIN; MATEUS S. ANGELO; STEFANO O. SOUZA; DOUG GEISLER; DANTE MINNITI; ROBERTO SAITO; LILIA P. BASSINO; BRUNO J. DE BÓRTOLI; ANDRÉ FIGUEIREDO; LEANDRO RÍMULO

Bologna

Simposio; Star Clusters: from the Milky Way to the Early Universe; 2019

The VISCACHA (VIsible Soar photometry of star Clusters in tApii and CoxiHuguA?) Survey is an ongoing project based on deep and spatially resolved photometric obser-vations 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>300hof telescope time to observe∼150 star clusters, mostly with low mass (M <104M) on theoutskirts of the LMC and SMC. With this high-quality data set, we homogeneously determinephysical properties using deep colour-magnitude diagrams (ages, metallicities, reddening, dis-tances, 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 Magel-lanic Clouds and their evolution. We present the VISCACHA survey and its initial results, basedon our first two papers. The project?s long term goals and expected legacy to the communityare also addressed.