Speaker: Chris D’Andrea
Location: Institute of High Energy Physics, Beijing
A description of the survey strategy, spectroscopic program, and cosmological predictions for the Dark Energy Survey (DES) Supernova Survey. Additionally, we briefly discussion potential synergies of DES Supernova with the KDUST pre-curser, the Antarctic Survey Telescope 3, which will perform a very large area low-redshift survey.
This talk was given as part of the KDUST Workshop, Institute of High Energy Physics, Beijing, Nov 7-9, 2011