This Hubble Space Telescope Treasury program is imaging 50 nearby galaxies in full color resolving many of their stars, star clusters and associations. Science goals: (1) quantify how the clustering of star formation evolves both in space and time, (2) discriminate among models of star cluster evolution, (3) investigate the effects of starformation history on the UV starfornation rate calibrations, (4) explore the impacts of environment on star formation and cluster evolution across the full range of galactic and ISM properties, (5) investigate UV-excess globular clusters across multiple environments, (6) study the environment surrounding supernovae.
Description of the survey (Calzetti et al. 2014 accepted for publ. in AJ). Link to LEGUS website.