Legacy ExtraGalactic UV Survey (LEGUS) with The Hubble Space Telescope.
  I. Survey Description
  The Legacy ExtraGalactic UV Survey (LEGUS) is a Cycle 21 Treasury program on
the Hubble Space Telescope, aimed at the investigation of star formation and
its relation with galactic environment in nearby galaxies, from the scales of
individual stars to those of ~kpc-size clustered structures. Five-band imaging,
from the near-ultraviolet to the I-band, with the Wide Field Camera 3, plus
parallel optical imaging with the Advanced Camera for Surveys, is being
collected for selected pointings of 50 galaxies within the local 12 Mpc. The
filters used for the observations with the Wide Field Camera 3 are: F275W(2,704
A), F336W(3,355 A), F438W(4,325 A), F555W(5,308 A), and F814W(8,024 A); the
parallel observations with the Advanced Camera for Surveys use the filters:
F435W(4,328 A), F606W(5,921 A), and F814W(8,057 A). The multi-band images are
yielding accurate recent (<~50 Myr) star formation histories from resolved
massive stars and the extinction-corrected ages and masses of star clusters and
associations. The extensive inventories of massive stars and clustered systems
will be used to investigate the spatial and temporal evolution of star
formation within galaxies. This will, in turn, inform theories of galaxy
evolution and improve the understanding of the physical underpinning of the
gas-star formation relation and the nature of star formation at high redshift.
This paper describes the survey, its goals and observational strategy, and the
initial science results. Because LEGUS will provide a reference survey and a
foundation for future observations with JWST and with ALMA, a large number of
data products are planned for delivery to the community.
