Legacy ExtraGalactic UV Survey (LEGUS) with The Hubble Space Telescope. I. Survey Description
Abstract
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.
Keywords
Cite
@article{arxiv.1410.7456,
title = {Legacy ExtraGalactic UV Survey (LEGUS) with The Hubble Space Telescope. I. Survey Description},
author = {D. Calzetti and J. C. Lee and E. Sabbi and A. Adamo and L. J. Smith and J. E. Andrews and L. Ubeda and S. N. Bright and D. Thilker and A. Aloisi and T. M. Brown and R. Chandar and C. Christian and M. Cignoni and G. C. Clayton and R. da Silva and S. E. de Mink and C. Dobbs and B. G. Elmegreen and D. M. Elmegreen and A. S. Evans and M. Fumagalli and J. S. Gallagher and D. A. Gouliermis and E. K. Grebel and A. Herrero and D. A. Hunter and K. E. Johnson and R. C. Kennicutt and H. Kim and M. R. Krumholz and D. Lennon and K. Levay and C. Martin and P. Nair and A. Nota and G. Oestlin and A. Pellerin and J. Prieto and M. W. Regan and J. E. Ryon and D. Schaerer and D. Schiminovich and M. Tosi and S. D. Van Dyk and R. Walterbos and B. C. Whitmore and A. Wofford and .},
journal= {arXiv preprint arXiv:1410.7456},
year = {2015}
}
Comments
67 pages, 9 figures; accepted for publication on the Astronomical Journal